The galaxy presents a predominantly smooth morphology. A central bulge region is evident, displaying a concentrated luminosity gradient, suggesting a significant population of older stars. Fainter, more diffuse light extends outwards from the bulge, giving the galaxy an elliptical appearance. The galaxy appears to be mostly smooth, and while some minor irregularities are present, there is no readily apparent structure. There is a very slight hint of asymmetry, but no clear evidence of tidal features or ongoing major mergers. The color profile suggests a relatively evolved stellar population.
