The galaxy exhibits an overall elliptical morphology, appearing generally smooth and centrally concentrated with no readily apparent spiral arm structure. The light distribution suggests a more or less spheroidal shape, with a bright, possibly slightly elongated core region. The galaxy presents with a color gradient, appearing more yellow/white at the core and gradually transitioning to a bluer hue towards the outer edges. There are no distinct features such as dust lanes, prominent star-forming regions, or tidal tails immediately visible. No signs of major galactic mergers are obvious, though a subtle distortion or faint, extended emission may potentially indicate minor gravitational interactions or past mergers. Overall, the galaxy appears to be a relatively quiescent system without significant ongoing star formation in its outer regions.
