The galaxy presents as a somewhat elliptical, though not perfectly symmetrical, structure. There is a noticeable central bulge that appears yellowish-white, suggesting an older stellar population concentrated towards the galaxy's core. The galaxy exhibits a faint, diffuse disk surrounding the central bulge. The disk is composed of a mix of colors, with a faint bluish tinge in some regions indicating the presence of younger, hotter stars and ongoing star formation, though this appears to be occurring at a fairly low rate. There is some irregular structure within the disk, but it is not obviously indicative of a major ongoing merger event. Overall, the galaxy seems to be relatively smooth in appearance, with no prominent spiral arms or strong tidal features. 
