The galaxy presents as a slightly elongated, elliptical structure. The central bulge exhibits a concentrated, high-luminosity profile, appearing a warmer color indicating an older stellar population. Moving outward from the core, the galaxy displays a smooth luminosity gradient, transitioning to a more diffuse halo. The overall color appears to be trending towards redder hues, suggesting moderate levels of star formation or a population dominated by evolved stars. There are no obvious signs of spiral arms, rings, or prominent dust lanes. There may be some tidal features present, although they are faint and do not substantially disrupt the galaxy's overall smooth morphology. The galaxy appears relatively isolated, with no apparent close companions or ongoing major interactions.
