The galaxy presents as a single, somewhat diffuse object, though there may be an ongoing merger. There appears to be a primary, larger component, with a slightly less luminous, secondary component exhibiting a more reddish hue. The galaxy's overall morphology leans towards being smooth in appearance, lacking distinct spiral arms or a prominent disk structure. The shape is intermediate between round and elongated. A degree of disturbance is present, suggesting potential tidal interactions. There is a possibility of a merger event in progress. The central region appears more concentrated in luminosity. The primary component seems to have a larger extent. The color index indicates ongoing star formation activity within the galaxy, although the smoother appearance suggests a transition phase where star formation may be declining in some regions.
