The galaxy presents an overall smooth morphology, with a centrally concentrated light profile that diffuses outwards. It appears largely elliptical in shape, exhibiting a moderate degree of roundness rather than a highly elongated, cigar-like structure. There is a slight suggestion of an extended disk-like structure but is difficult to tell with certainty from this view.

Color gradients are observable within the galaxy. The central region exhibits a more yellow hue, potentially indicating an older stellar population. The outer regions are slightly bluer.

There is some indication of disturbances or minor tidal features present, which may be due to an ongoing or past merger event. These appear as subtle asymmetries and faint extensions. These disturbances may indicate a period of active star formation, although the galaxy is not displaying a significantly high star-forming rate.
