The galaxy presents a roughly elliptical morphology, though its disk is not well resolved. It appears to be an edge-on or highly inclined spiral galaxy. The central region exhibits a higher concentration of luminosity, suggesting the presence of a bulge. The color gradient shows bluer tones, possibly indicating ongoing or recent star formation. There are potential signs of minor disturbances, hinting at tidal interactions or past merger events. While the galaxy does not appear to be undergoing a major merging event, some asymmetry is visible within its overall structure. There may be some fainter, diffuse features extending outwards from the main body, which could be tidal tails or debris from interactions. Overall, the galaxy seems to be an active system with a moderate amount of star formation and a somewhat disturbed morphology.
