The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, approaching circular. The color profile is predominantly yellow, suggesting an older stellar population. There is no apparent spiral structure or evidence of active star formation regions discernable in the image. There are no indications of tidal tails or significant morphological disturbances, suggesting it is not undergoing a major merger, although a very subtle asymmetry could imply a minor interaction. The light is concentrated in the center, but slowly diffuses outwards, indicating a possible halo. Overall, the galaxy appears to be a mature system with a large stellar mass and little current star formation.
