The galaxy presents a predominantly smooth morphology. It exhibits an elliptical shape, appearing slightly elongated, and generally features an ellipsoidal structure. The central bulge is clearly visible and relatively bright, with a yellowish hue suggesting a population of older stars. There is little evidence of strong spiral arm structures or prominent dust lanes. The outer regions of the galaxy fade gradually into the background sky. The lack of prominent blue regions indicates a low rate of ongoing star formation. There appears to be a hint of minor disturbance, perhaps indicating a small gravitational interaction or past merger.
