The galaxy presents as a moderately bright, elliptical morphology. The light distribution appears relatively smooth, with a central concentration that fades gradually outwards. No distinct spiral arms or bar structures are readily apparent. The galaxy's color profile indicates a redder overall hue, suggesting a population of older stars and a lower rate of on-going star formation. There is a slight suggestion of bluer regions, possibly indicating pockets of younger stars, however, the overall smooth appearance suggests this is unlikely. The galaxy appears somewhat disturbed; while no major signs of merging are visible, a minor disturbance cannot be ruled out. The estimated size indicates this is a moderately sized galaxy.
