The galaxy presents as a single, relatively symmetrical object. It exhibits a centrally concentrated luminosity profile, suggestive of an elliptical or lenticular galaxy morphology. The core region displays a pronounced yellow hue, which may indicate an older stellar population and reduced ongoing star formation. The outer regions of the galaxy appear to fade gradually into the background, exhibiting a smooth transition without any obvious spiral arm structure or irregular features. There are no obvious signs of tidal disturbances, strong dust lanes, or recent merger activity in the immediately visible structure, pointing towards a dynamically relaxed system.
