The galaxy presents as a primarily smooth object, with a noticeable elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The light distribution is concentrated towards the center, indicating a prominent galactic bulge. The galaxy appears to be in a relatively isolated environment, with no obvious signs of major tidal interactions or ongoing mergers, though a slight asymmetry could suggest a minor past interaction. The color gradient suggests an older stellar population, with a redder hue dominating the central regions, transitioning to slightly bluer tones in the outer regions. The overall color suggests moderate levels of star formation.
