The galaxy appears to be an elliptical galaxy exhibiting a predominantly smooth morphology. The light distribution suggests a high degree of radial symmetry, with a centrally concentrated bulge. The galaxy displays a yellowish hue in the center, gradually transitioning to a bluish color towards the outer regions. This color gradient suggests a difference in the stellar populations, where the central bulge might be dominated by older, redder stars, while the outskirts contain some younger, bluer stars. There is some indication of minor disturbances or faint tidal features that are a hint of possible past interaction events. The galaxy's overall structure is relatively compact and moderately luminous. The slight elongation suggests it is closer to round rather than cigar-shaped. No distinct spiral arms or prominent dust lanes are visible. Overall, the galaxy appears to be a fairly evolved system.