The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. The light is concentrated towards the center, indicating a dense stellar population in the core. The galaxy has a generally round shape, with no apparent spiral arms or bar structures. There is a slight color gradient from the center outwards, with the core exhibiting a yellower hue, suggesting an older stellar population dominating this region. The outer regions have a slightly bluer tint, possibly indicating the presence of younger stars, although star formation rates are very low. There is no evidence of active galactic nuclei or significant dust lanes obscuring the galaxy's light. The galaxy does not show signs of any major recent mergers, although there is evidence to suggest minor disturbances or tidal interactions in its past. Overall, this galaxy presents as a well-formed, evolved system undergoing little or no active star formation.
