This galaxy presents a predominantly smooth morphology, appearing elliptical or lenticular in shape. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in luminosity towards the outer regions. The core is a brighter yellow, which may indicate an older stellar population compared to the fainter, redder outer regions. There's no clear evidence of spiral arms or significant dust lanes. Overall, the structure is relatively undisturbed, showing no prominent signs of ongoing or recent major mergers, but there is a potential minor visual disturbance. The galaxy's overall appearance indicates a high probability of a classification as a spheroidal or elliptical galaxy.