The galaxy presents as a roughly elliptical form, with a moderate degree of elongation along its major axis. The color profile suggests a population dominated by older stars, exhibiting a yellowish hue, particularly concentrated toward the central bulge. There is a subtle bluer component present, possibly indicative of ongoing, though relatively subdued, star formation. No clear spiral arm structure is discernible. The overall morphology appears relatively undisturbed, lacking significant signs of tidal interactions or recent mergers. The galaxy's light profile suggests a smooth transition in stellar density from the core outward, with no sharp discontinuities or rings immediately apparent. It seems to reside in a relatively quiescent state, based on the observed features.
