The galaxy presents as a centrally concentrated, elliptical morphology, exhibiting a smooth light distribution. The core displays a bright, yellowish hue, indicative of an older stellar population. The overall shape appears primarily round, though closer examination reveals some deviation. There is a subtle flattening, indicating a potential transition between elliptical and lenticular morphology. Faint wisps of extended, diffuse light surround the brighter central region, gradually fading into the background sky. These features suggest a relatively quiescent galaxy, with moderate star formation activity. Subtle disturbances may be present in the outer regions, but there is no clear evidence of major ongoing mergers or strong tidal interactions.