The galaxy appears as a centrally concentrated, luminous structure. It is fairly smooth in appearance, with a slight elongation suggestive of a possible elliptical morphology. The color profile is predominantly yellow/orange, indicating an older stellar population. There is little evidence of significant dust lanes or prominent spiral arm structures. The overall appearance suggests a galaxy undergoing relatively little active star formation at this time. There are no obvious signs of major disturbances such as tidal tails or other features indicative of a recent major merger event, though a subtle asymmetry or minor disturbance cannot be ruled out given the image quality. The estimated size is relatively compact.
