This galaxy appears to be a relatively smooth, elliptical-like structure. The light profile seems to gradually diminish from the center outwards, lacking any prominent spiral arms or distinct features. There is a slight elongation, possibly transitioning towards a cigar shape, but overall it maintains a predominantly rounded appearance. The color distribution suggests a population of older stars. A subtle blue tinge is present, indicating some ongoing, low-level star formation, though the dominant stellar population appears to be older. There is no obvious evidence of major mergers or strong tidal disturbances in the image. The galaxy seems to be a relatively isolated system, with no closely interacting companions visible.
