This galaxy exhibits a predominantly smooth morphology. The central region is characterized by a bright, concentrated bulge displaying a yellowish-white hue, suggesting a population of older stars. Surrounding the central bulge is a more diffuse, extended halo. There are faint hints of bluer light extending outward from the core, possibly indicating some regions of ongoing star formation, though the overall color profile suggests a relatively low star formation rate compared to other galaxies. The shape appears to be in between round and elliptical. There is no apparent tidal disruption or nearby galaxies causing it to go through a major disturbance. This galaxy displays no apparent signs of a major merger event or significant morphological disturbance.
