The galaxy presents as a centrally concentrated object. It is roughly elliptical in shape, though not perfectly symmetrical, exhibiting some subtle irregularities in its outer isophotes. The core region appears bright and compact, indicating a likely concentration of older stellar populations.

The color gradient suggests a gradual reddening towards the central region of the galaxy, consistent with an increasing age and metallicity of the stars in that region. There is no clear evidence of spiral arm structure or prominent dust lanes. There might be slight disturbances in the morphology which indicate the possibility of a recent or ongoing minor merger event. The overall smooth appearance suggests a classification as an elliptical galaxy.
