The galaxy presents as a smooth, elliptical-like object, exhibiting a concentrated central bulge. The light distribution appears relatively uniform across the galaxy, with a gradual decrease in brightness from the core outwards. The shape is elongated, displaying an "in between" roundness, with no distinct spiral arms or disk structures visible. There are no obvious signs of ongoing major merging activity or significant disturbances in the overall structure, though some minor disturbances cannot be ruled out. Its colouration suggests a population of older stars, with a reddish/yellow hue dominating. A relatively low rate of star formation is anticipated, based on the smooth morphology and colour. The galaxy's estimated size is relatively small, considering the estimated mass of the galaxy.
