The galaxy presents as a relatively smooth and concentrated object. Its overall shape is elliptical, appearing almost perfectly round. The luminosity profile suggests a dense central bulge that gradually fades outward toward its edges. There is a lack of any distinct spiral arm structure. The color appears to be generally uniform across the galaxy, with a slight tendency toward redder hues. There is no evidence of active star formation regions. Based on its morphology, it appears to be a galaxy undergoing relatively little interaction. Small indications of a possible minor disturbance are present.
