The galaxy appears to be a relatively smooth object, exhibiting an elliptical morphology. The light distribution suggests a spheroid-dominated system with a noticeable concentration of light towards the center, which appears yellowish. This could indicate a population of older stars dominating the core. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be mostly unperturbed, with no obvious signs of major mergers or tidal disruptions, though there is potentially some minor distortion in the outer regions of the galaxy. It has a moderate size relative to other objects in the field. The color gradients suggest that star formation is either suppressed or primarily occurring in the core region.
