The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in surface brightness moving outwards. There is no evidence of spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. The dominant color is a yellowish-orange hue, suggestive of an older stellar population. The galaxy appears largely undisturbed, without any obvious signs of tidal interactions or merging events. It displays a fairly round shape, with no significant elongation. Any internal structure is unresolved at this scale.
