The galaxy presents a primarily smooth morphology, with a general elliptical shape. It exhibits a concentrated central bulge, with light gradually fading towards the edges, indicating a lack of prominent spiral arms or distinct disk features. The central region appears yellowish, possibly indicative of an older stellar population. Fainter blue fringes may point towards a younger star formation, though they are diffuse and limited. There is little indication of recent major merger activity or significant morphological distortions in the galaxy's structure.
