The galaxy presents as a moderately luminous spiral system with a redshift of approximately 0.045, indicative of its cosmological distance. The galaxy exhibits a complex morphology. The disk component is clearly visible, displaying distinct spiral arm structures. These arms show signs of active star formation, evidenced by the presence of bluer regions interspersed within the spiral pattern. The central bulge of the galaxy appears to be of moderate size and exhibits a yellowish hue, possibly indicating an older stellar population with reduced star formation activity compared to the disk. There is evidence of significant gravitational interaction or ongoing merger activity. The overall structure appears disturbed, with asymmetric features that deviate from a classic spiral morphology. This disturbance likely influences the distribution of stars and gas within the system. The shape of the main galaxy body seems elongated, potentially indicating the presence of tidal tails or distortions due to the gravitational forces at play. There appears to be an interacting nearby component, this could indicate ongoing or recent merger activity. 