The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The overall shape is elliptical, trending towards a more oblate form rather than a highly elongated one. There is a hint of an extended component, possibly a faint halo or tidal feature, though this is subtle. The color gradient suggests a redder core region, which could indicate an older stellar population, with a slight shift towards bluer tones in the outer regions, potentially signifying some level of recent star formation. There is no obvious spiral structure or bar visible. There are possibly some minor distortions visible in the outer regions of the galaxy, which may suggest a history of minor mergers or tidal interactions.
