The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. It possesses a generally round morphology, with minimal evidence of spiral arms or a prominent disk structure. The galaxy's core region displays a bright, concentrated luminosity, suggesting a high density of stars. The overall color of the galaxy leans towards the red end of the spectrum, indicative of an older stellar population and a relatively low rate of ongoing star formation. There is no clear indication of significant tidal disturbances or major mergers in its recent history, although a slight asymmetry in its outer isophotes hints at possible minor interactions or past merger events. 
