The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The core exhibits a pronounced yellowish-orange hue, suggestive of an older stellar population dominating its composition. Moving outwards from the core, the color gradually shifts towards a redder, fainter halo. This could indicate a decrease in metallicity or a change in the age distribution of the stellar populations within the galaxy's outer regions. There is no obvious evidence of spiral arms or a distinct disk-like structure. It appears relatively undisturbed, lacking any significant signs of tidal interactions or ongoing mergers. The shape tends more towards an elliptical shape with a small cigar shape, rather than a perfectly circular form. Overall, the galaxy appears to be a relatively quiescent system, potentially a massive elliptical galaxy with a substantial population of evolved stars.
