The galaxy presents a primarily smooth morphology, appearing largely spheroidal in shape. It exhibits a concentrated central bulge which dominates the overall light profile. There's subtle evidence of a possible faint disk component that extends from the central bulge. The color of the galaxy appears to be leaning towards the redder side of the spectrum, indicating a likely older stellar population with a lower rate of star formation. There is a potential minor disturbance, perhaps indicative of an interaction. It's possible this is related to the other galaxy that is near it.
