The galaxy appears to be elliptical or lenticular in morphology, with a relatively smooth and featureless structure. It is generally round in shape with a moderate size. The central region exhibits a higher concentration of light, fading towards the outer edges. There is no clear evidence of spiral arms or a well-defined disk component. There are no indications of any major mergers or strong tidal disturbances, though some minor disturbances could be present. The color gradient suggests an older stellar population. Overall, it is a quiescent galaxy with low levels of star formation.
