The galaxy presents as a roughly elliptical, centrally concentrated object. The core exhibits a bright, yellow-tinged luminosity, suggesting a population of older stars. The isophotes appear mostly smooth, with a subtle extension of light in one direction giving it a slightly elongated appearance. There are hints of bluer light in the outer regions, possibly indicating some ongoing star formation within the galaxy, though it appears to be a relatively small proportion of the overall light output. There is no obvious indication of strong spiral arm structure or a prominent disk, nor are there any readily apparent signs of a major ongoing merger or tidal disturbance, although subtle asymmetries cannot be ruled out based on this image alone.
