The galaxy presents as an elliptical system with a relatively smooth and concentrated luminosity profile. The central region exhibits a bright, yellowish-white core, suggestive of an older stellar population. Moving outward from the core, the light gradually fades into a less concentrated, more diffuse halo with a slightly bluer tinge, indicating the possible presence of younger stars or a different stellar population. The galaxy appears to be somewhat flattened and elongated. There is no visible evidence of spiral arms, dust lanes, or ongoing major merger activity. The overall appearance suggests a galaxy that is relatively evolved and quiescent in terms of star formation, with a dominant spheroidal component.
