The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. It appears nearly circular but shows a slight elongation. The central region is bright and yellowish, suggesting an older stellar population. Fainter, bluer colors are subtly visible in the outer regions, potentially indicative of more recent star formation. The galaxy lacks any apparent spiral arm structure or significant dust lanes. Overall, it appears to be a relatively quiescent galaxy dominated by older stars, with limited ongoing star formation.
