The galaxy presents an elliptical morphology, with a smooth light distribution and no apparent spiral arm structures. The central region exhibits a high concentration of light, gradually decreasing outwards. Its overall color appears to be slightly yellowish, suggesting a population of older stars with relatively low ongoing star formation. The galaxy appears somewhat elongated, with a slight tilt relative to the line of sight. There is no evidence of significant disturbances or tidal features, suggesting it is likely a relatively isolated system or has completed the merging process some time ago. There is some evidence of bluer light in some spots indicating areas with slightly more star formation.
