The galaxy presents an overall smooth morphology with a slight elongation. It appears nearly elliptical in shape, exhibiting a gradual decrease in luminosity from the central region outward. The color profile suggests an older stellar population, indicated by the redder hues concentrated toward the core, with slightly bluer regions at the periphery. There is no obvious spiral arm structure, dust lane, or any significant evidence of recent or ongoing major mergers. The central bulge seems well-defined. Slight asymmetry may be present at the edges, indicating a possible minor disturbance.
