The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge, which appears to be a dominant feature of its overall morphology. The color profile is yellowish, possibly indicating an older stellar population, or significant dust obscuration. There is very little evidence of spiral arm structure. The galaxy appears to be relatively undisturbed, with no obvious signs of recent or ongoing major mergers. There might be hints of a minor tidal interaction or a weak feature emanating from the galaxy, but this is not definitively resolved. The overall shape tends towards being round, and the light distribution suggests a centrally concentrated object.
