The galaxy presents as a moderately compact, elliptical structure. It appears relatively smooth in morphology, with a gradual change in surface brightness from the core outwards. There is no readily discernible disk component, spiral arm structure, or significant dust lane. The galaxy exhibits a yellowish-red hue, indicative of an older stellar population with lower levels of recent star formation. The overall shape suggests a spheroidal morphology, leaning slightly toward a flattened, oblate spheroid rather than a perfect sphere. Close inspection reveals hints of a faint, extended halo surrounding the main body of the galaxy. No signs of ongoing major merger events are evident, although there's a possibility of minor tidal disturbances.
