The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There is a distinct lack of resolved features such as spiral arms or a prominent disk structure. The central region displays a bright, somewhat diffuse glow, suggesting a possible active galactic nucleus or a high concentration of older stars. The galaxy's color appears to be slightly redder than average, potentially indicating an older stellar population with reduced ongoing star formation. There's no apparent dust lane obscuring the galactic center or any signs of recent merger activity or tidal disturbances that could be indicative of interaction with other galaxies. The overall form indicates this is likely a relatively massive galaxy that has largely completed its period of major star formation.
