The galaxy presents a largely elliptical morphology. It appears as a diffuse, centrally concentrated object with a smooth light profile, suggesting a relatively old stellar population. There is little evidence of spiral arms or dust lanes. The overall color is somewhat red, indicating the presence of older stars and a lower rate of ongoing star formation. The galaxy exhibits a high degree of central concentration and circularity, showing no signs of significant tidal disturbances or recent merger activity. It appears to be an isolated system with minimal interaction with neighboring galaxies.
