The galaxy presents as a single, relatively smooth object with a near-circular morphology. There is a slight elongation, but the overall shape leans towards rounded rather than cigar-shaped. The galaxy exhibits a primarily smooth structure, with only subtle hints of internal features. Light distribution appears concentrated towards the center. There is no discernible spiral arm structure or prominent disk component. The color gradient suggests the possibility of an older stellar population, as indicated by the somewhat redder hue of the galaxy. There are slight hints of interaction or minor disturbance around the galaxy, but there is no obvious major merging event in progress. The image hints that the galaxy might be interacting with another nearby object but more imaging is required to determine a definitive link.
