The galaxy presents a largely smooth, elliptical morphology. It appears as a centrally concentrated spheroid with a gradual decrease in luminosity from the core to the outer regions. The color profile indicates a population of older stars, exhibiting a yellow to reddish hue in the central bulge, suggesting lower levels of ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears to be relatively isolated with no immediate signs of major tidal disturbances or ongoing mergers, though a slight asymmetry may indicate a minor past interaction. The overall shape is predominantly rounded, transitioning smoothly from the bright core to the fainter surrounding halo.
