The galaxy presents as a moderately concentrated object with an elliptical morphology. It exhibits a relatively smooth texture in the central region, with a subtle elongation along its major axis. There appears to be some level of disturbance. There may be a merging partner that is causing this, and that merging may not yet be complete. The galaxy displays a yellowish-orange hue. This color suggests a stellar population dominated by older, redder stars. The overall appearance indicates a system that might be undergoing some merging. The object shows a well-defined central region, but there also appear to be less-defined features and irregularities that could indicate either tidal debris or the influence of nearby galaxies.
