The galaxy appears to be a relatively smooth and elliptical-shaped object. It exhibits a dominant central bulge that appears quite bright, with a yellowish hue suggestive of an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. The overall color suggests a relatively passive galaxy, potentially with a low rate of star formation. It is moderately sized, and shows no indications of any major disturbances or ongoing mergers in this image, and has a seemingly regular morphology. The galaxy’s profile is mostly round, rather than elongated.
