The galaxy presents a generally smooth morphology with a dominant, centrally concentrated bulge. This central region exhibits a yellowish-orange hue, possibly indicative of an older stellar population. The galaxy's shape appears to be somewhere between round and elliptical. There is no apparent disk structure or spiral arm features. The galaxy appears largely undisturbed, without any obvious signs of ongoing major mergers or tidal disruptions, however there is a slight asymmetry to its morphology and/or some minor disturbances may be present. It has a moderate size for a galaxy at its distance. There's a hint of bluer light extending from the central bulge, indicating the presence of a younger stellar population and possible ongoing, though likely low, star formation activity.
