This galaxy presents as a singular, largely homogenous object. It displays a general spheroid shape with a smooth, featureless morphology. A high degree of central concentration is observed, with a gradual decline in luminosity from the core outwards. The light profile suggests minimal substructure or distinct spiral arms.

The color index suggests a galaxy dominated by an older stellar population, exhibiting a redder overall hue. Subtle asymmetry is present, potentially indicative of a past minor interaction or ongoing tidal disturbance, though no major distortions are apparent. There may be signs of early merging in the galaxy's outskirts. However, this is not a full-blown merger and appears to only show a disturbance.

The estimated size indicates a substantial galaxy, consistent with a high stellar mass. Star formation appears to be suppressed. Overall, this galaxy appears to be a massive, evolved system with signs of past interaction or potential ongoing disturbances.
