The galaxy presents a generally elliptical morphology with a relatively smooth light distribution. The central region exhibits a higher concentration of luminosity, appearing as a bright, slightly reddish core. Moving outward, the galaxy gradually fades into a diffuse halo. The overall color suggests a galaxy that has experienced significant stellar evolution. The disk appears face on. There is a slight asymmetry and hints of tidal features in the outer regions, potentially indicating a past minor interaction or merger event. The galaxy exhibits an overall bluish tint, indicative of a population of young, hot stars.
