The galaxy presents as a centrally concentrated object with a generally elliptical morphology. A prominent, bright, and somewhat diffuse bulge dominates the central region, exhibiting a yellowish-white color, likely indicative of an older stellar population. There's evidence of a fainter, more diffuse disk surrounding the bulge, characterized by a bluer hue, possibly indicating the presence of younger stars and ongoing star formation. However, the disk does not display clear spiral arm structures. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. It exhibits a smooth appearance. There are also no dust lanes apparent.
