The galaxy presents a generally smooth morphology, exhibiting a bright central bulge that gradually fades into the outer regions. The overall shape appears to be somewhere between elliptical and lenticular, with no clear spiral arm structures visible. The color profile is slightly redder in the central bulge, possibly indicating an older stellar population, and shifts to a slightly bluer hue in the outer regions, hinting at ongoing, but subdued, star formation. There is no apparent evidence of major mergers or significant tidal disturbances; the galaxy seems relatively undisturbed. The lack of distinct features suggests a more evolved system, likely dominated by older stars in its core, though there are still younger stars in the outer reaches of the galaxy.
