The galaxy appears as a centrally concentrated, luminous object with a yellowish hue in the inner region transitioning to a redder periphery. The overall morphology is smooth and elliptical, with a high degree of central concentration. There is no discernable spiral arm structure or prominent dust lanes. Subtle disturbances appear visible in the outer halo, with some hints of tidal tails or disrupted morphology. The galaxy's shape appears generally round, although not perfectly spherical, with a slight elongation. Based on the color profile, the central region likely contains an older stellar population. Overall, the galaxy appears to be a massive, evolved system potentially undergoing minor interactions.
