The galaxy exhibits an elliptical morphology, appearing somewhat flattened. Its light distribution is centrally concentrated with a smooth profile, suggesting an older stellar population. The core is bright and yellow, indicating a population of older stars dominating the light emission in that region. There is a subtle color gradient visible moving outward from the center, with a slight blueing apparent in the outer regions. The galaxy appears to be relatively isolated with no major signs of recent disturbance or interaction. The image suggests a galaxy undergoing passive evolution.
