The galaxy presents a generally elliptical morphology with a smooth appearance. The central region exhibits a concentrated, luminous core. The light distribution appears fairly uniform without obvious spiral arm structures. There is evidence of a slight asymmetry, possibly indicating a minor tidal disturbance or interaction with another galaxy. The galaxy displays a redder color profile in the central regions, suggestive of an older stellar population, while the outer regions show slightly bluer tones indicating the presence of some younger stars. Overall the galaxy appears to be experiencing a moderate amount of star formation. The galaxy appears to be fairly massive. There is evidence of a minor merger or tidal disturbance. The galaxy appears to be relatively large, with a smooth and centrally concentrated light distribution. 
