The galaxy in the image appears to be a relatively smooth, elliptical galaxy. It exhibits a somewhat cigar-shaped morphology, with a slight elongation visible along one axis. The light distribution is concentrated towards the center, fading gradually towards the outer edges, indicating a centrally dominant spheroid component. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy is mostly smooth and there appears to be no significant ongoing merger activity or major disturbances affecting its structure. It displays a redder color, suggestive of an older stellar population and less active star formation.
