The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, displaying a near-spherical shape with no obvious spiral arm structure. A bright central bulge dominates the light profile, exhibiting a yellowish hue suggestive of an older stellar population. The outer regions of the galaxy fade gradually into the background, with only a subtle color gradient indicating a transition from the yellower central region to slightly bluer outskirts. There is no strong evidence of active star formation within the galaxy based on the image data; star formation is estimated to be very low. No signs of tidal disturbances or ongoing mergers are apparent. 
