This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. The core region is bright and has a yellowish color, indicating a population of older stars. Moving outwards from the core, the light intensity gradually decreases, with a redder hue in the outskirts suggesting a less active star formation rate. The galaxy presents with a slightly elongated shape, with its major axis being roughly twice the length of its minor axis. There is no evidence of spiral arms or a significant disk component. No signs of any major ongoing mergers are visible, although subtle irregularities might suggest minor disturbances or tidal interactions. The overall structure suggests a relatively evolved system with minimal recent star formation.
