The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a high degree of roundness. There is little evidence of spiral arms or a pronounced disk structure. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Fainter, somewhat redder areas extend outwards from the center, with the hint of bluer areas on the periphery, which could suggest some ongoing star formation, albeit at a low rate. No significant merging signatures or major disturbances are readily apparent in its structure. There is a suggestion of some minor disturbances, and the galaxy appears to be experiencing a period of quiescence in terms of its star formation activity.
