The galaxy appears to be a relatively smooth, elliptical-like object. It is elongated, presenting an intermediate axis ratio. The galaxy exhibits a centrally concentrated brightness profile, with luminosity decreasing steadily outwards from the core. There is little evidence of spiral arm structure, distinct star formation regions, or significant dust lanes. A slight asymmetry or minor tidal feature might be present on one side, possibly indicating a past interaction or minor disturbance, but could also be a background object. The primary color of the galaxy appears to be a pale green, suggesting a lack of substantial ongoing star formation, and a stellar population dominated by older, redder stars. The overall structure suggests a gravitationally relaxed system.
