The galaxy presents an overall smooth appearance with a discernible disk-like structure. It exhibits an elliptical shape, elongated along one axis. A central bulge is present, appearing brighter and more concentrated than the surrounding disk. The galaxy's color profile suggests a mix of stellar populations, with a possible trend towards bluer colors in the outer disk regions. There is no obvious evidence of strong spiral arm structure or significant dust lanes within the galaxy. The galaxy appears relatively isolated, with no immediate signs of tidal interactions or ongoing mergers. Small disturbances may be present.
