The galaxy appears to be a relatively smooth, elliptical galaxy with a bright central bulge. It exhibits a slightly elongated, cigar-like shape. There is minimal evidence of spiral arms or significant disk structure. The color profile suggests an older stellar population, with a reddish hue concentrated towards the core, indicating a high density of evolved stars. The outer regions are slightly bluer, hinting at a small degree of ongoing, but limited, star formation. No major signs of recent or ongoing mergers are visible, although there may be a slight asymmetry in the outer halo, possibly from a minor past interaction. The galaxy appears to be a fairly isolated system.
