The galaxy presents a largely smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in luminosity outward from the core. The galaxy appears nearly round in projection with a slightly yellowish hue, suggesting a population dominated by older stars with minimal ongoing star formation. The lack of distinct spiral arms or dust lanes further supports its classification as an elliptical or lenticular galaxy. There is no significant indication of any recent merger activity or tidal disturbances. Overall, the galaxy appears to be a relatively isolated, evolved system.
