The galaxy presents a generally smooth morphology, appearing as a single, concentrated light source. Its overall shape is quite round. There is no discernible spiral structure or bar present. The color profile suggests an older stellar population, with light emission weighted toward the redder end of the spectrum, evidenced by a yellowish central area. The galaxy appears relatively undisturbed, showing no signs of ongoing major mergers or tidal disruptions. There may be very minor disturbances, although not clearly evident from visual inspection.
