The galaxy presents as a moderately luminous object, exhibiting a somewhat smooth morphology. It appears to be in the process of merging, or experiencing some form of gravitational interaction, as evidenced by a faint tidal feature extending from the main body. The galaxy displays a slight elongation, diverging from a perfectly circular form, with a color profile suggestive of moderate star formation activity. There is a subtle color gradient from the center outwards, with a more concentrated yellow/red hue in the central region, indicating an older stellar population, while bluer fringes indicate ongoing or recent star formation. The overall structure seems to be undergoing significant disturbance due to the likely ongoing merger event.
