The galaxy appears to be relatively compact, with a noticeable bulge. Its overall form leans towards elliptical, exhibiting a smooth, symmetrical distribution of light. The central region displays a yellowish hue, perhaps indicative of an older stellar population, while the outer edges have a bluer tinge, hinting at the presence of younger stars or ongoing star formation activity. Some minor disturbances are present, though they are not as clear in the image. The main galaxy appears to be interacting with a smaller object, hinting at the possibility of an ongoing or recent merger event.
