This galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology. It shows a high degree of central concentration. The galaxy's light profile is highly concentrated towards the core, fading gradually outwards. The overall color appears relatively red, suggesting a population dominated by older stars and a lack of significant ongoing star formation. There is no evidence of spiral arms or a prominent disk component. No prominent dust lanes or other features that may indicate recent merger activity are apparent in this image. The galaxy shows little flattening and seems to be close to circular.
