The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical galaxy, appearing largely featureless without prominent spiral arms or a distinct disk structure. The light profile is relatively smooth, with a gradual decrease in luminosity from the core outwards. The central region exhibits a yellowish hue, which may indicate an older stellar population dominating the core. Fainter, bluer light surrounds the central bulge which could point to a small amount of younger stars and potentially ongoing star formation. There is no evidence of any major disturbances or mergers.
