The galaxy appears as a relatively small, elliptical structure, exhibiting a smooth and centrally concentrated light distribution. The color profile suggests a lack of significant ongoing star formation, with a bluer core transitioning to redder outer regions. There is no discernible spiral arm structure or prominent dust lanes. The overall shape is somewhat elongated but generally round, and there are hints of minor disturbances or interactions with smaller companion galaxies, but they are very weak. It is a well-defined object with a relatively uniform light profile.
