The galaxy presents as a generally smooth, centrally concentrated object. Its overall shape approximates a rounded form, though some irregularity is apparent in the isophotes. A faint disk-like structure may be present, but this is difficult to ascertain definitively.

Color gradients are observed within the galaxy. The central region exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the center, a subtle shift towards bluer colors is noted, hinting at the presence of younger stars in the outer regions.

There are faint indications of minor disturbances in the galaxy's morphology. The light distribution is not perfectly symmetrical, with a slight extension or asymmetry visible on one side, possibly related to a past or ongoing interaction. However, no prominent tidal features or signs of a major merger are evident.
