The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that transitions into a more diffuse outer halo. The color profile suggests an older stellar population, with the central region displaying a yellowish-orange hue, indicative of aging stars and a low rate of ongoing star formation. The overall shape is somewhat rounded, with only a slight deviation from perfect circularity. There is no apparent evidence of spiral arms, dust lanes, or any major disturbances suggestive of recent or ongoing mergers with other galaxies. The galaxy is a relatively compact system.
