The galaxy presents a generally smooth morphology, though subtle features are observable. The primary structure appears spheroidal with a bright central bulge. There is an apparent extension, or potential tidal tail, emanating from the main body, suggesting a gravitational interaction or past merger event.

The color gradient indicates a population shift, with the central bulge exhibiting a more yellow/orange hue, which could represent an older stellar population. The extended feature is slightly redder. The galaxy shows an approximately round shape, although subtle asymmetries are present. Evidence for substantial dust lanes or active star formation regions are not readily apparent from the data.
