The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions smoothly into an extended halo. The core of the galaxy is bright, suggesting the presence of a significant stellar population or active galactic nucleus. There is a slight color gradient within the galaxy, with the central region appearing more yellow/orange and the outer regions appearing more red, suggesting a difference in the age and composition of the stellar populations. No obvious spiral arms or disk-like structures are apparent, and there is no evidence of ongoing major mergers or tidal disturbances. Given its high mass estimate, the galaxy is likely a massive system. The galaxy's low star formation rate aligns with the morphological classification of an elliptical, indicating a population dominated by older stars.
