The galaxy presents as a relatively smooth object, with a slight elongation. There appears to be a brighter, concentrated central region, possibly indicative of a galactic bulge or active galactic nucleus. The galaxy displays a color gradient, shifting from bluer tones near the center to more reddish hues in the outer regions. There is a faint hint of a disk-like structure with some subtle irregularities, suggesting a possible spiral or disturbed morphology, although a significant portion of the light is distributed smoothly. Overall, the galaxy is an intermediate-mass galaxy with evidence of low to moderate star formation rates and a red shift of approximately 0.178. The galaxy is likely experiencing minor gravitational disturbances due to the asymmetry in its shape and the diffuse features in the outer regions.
