The galaxy appears to be a relatively smooth, elliptical-like object with a concentrated central bulge. It exhibits a fairly symmetrical morphology. The color gradient suggests a population of older stars, particularly in the central region, which displays a yellowish hue. Fainter, more diffuse blue light extends outwards, suggesting regions of possible ongoing, albeit low, star formation activity in the outer areas. There is only minimal visual evidence of spiral arms or distinct morphological features such as bars or rings, supporting its classification as likely an early-type galaxy. There's no indication of major mergers, but there might be some slight disturbance.
