The galaxy presents as a moderately sized, elliptical morphology. Its central region exhibits a high concentration of luminosity, appearing smooth and relatively featureless. There is a gradual decline in brightness towards the outer edges, with no distinct spiral arms or bar structures visible. The overall color appears slightly redder, indicative of a population dominated by older stars and lower star formation rates. The galaxy displays a somewhat rounded shape. There may be minor distortions present, but there's no definitive evidence of a major ongoing merger or tidal disturbance.
