The galaxy presents a largely smooth morphology, with a centrally concentrated, bright, and yellowish core. The overall shape is somewhat elliptical, appearing relatively round in projection. There is little evidence of spiral arm structure or significant dust lanes. The light distribution suggests a relatively uniform stellar population with the core being older, with little to no ongoing star formation. There is a very faint and diffuse halo surrounding the central region, gradually fading into the background sky. The galaxy does not appear to be undergoing any major merging events. Faint hints of minor disturbances are seen around the galaxy's edge. The estimated size appears moderate in relation to other galaxies in the observed field.
