The galaxy appears as a relatively smooth, elliptical-like object. Its overall shape is somewhat elongated, but not significantly so; it seems to be trending towards a more spherical morphology. The color profile exhibits a central concentration of reddish-yellow light, suggesting an older stellar population dominating the core. The outer regions appear bluer, hinting at the presence of some younger, though likely limited, star formation. There is no strong evidence of a distinct disk structure or spiral arms, and it seems to be in a relatively relaxed state, with no signs of ongoing major mergers or significant tidal disturbances. However, there is a faint hint of some asymmetry which may indicate a minor disturbance or past interaction.
