The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a noticeable radial decrease in luminosity moving outward. The color appears to be generally yellowish-orange, suggestive of an older stellar population and relatively low levels of current star formation. There is no discernible spiral arm structure or dust lane features visible at this resolution. The galaxy appears largely undisturbed, with no apparent signs of major merger activity or significant tidal interactions. It appears somewhat lenticular when considering the shape and smooth features.
