The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The light profile suggests a general spheroidal morphology. The galaxy exhibits a yellow-orange hue, indicative of an older stellar population with fewer young, blue stars. There is no visible spiral arm structure or significant dust lane obscuration. The galaxy's shape is more rounded than elongated. No tidal tails or other obvious signs of recent major merger activity are apparent, though there is a minor disturbance nearby. The overall appearance is consistent with a galaxy undergoing passive evolution, having largely exhausted its gas supply for star formation, resulting in a population of older, redder stars.
