The galaxy appears as a single, relatively smooth, elliptical-like object. It exhibits a concentrated central bulge with a notable decrease in luminosity as one moves outward from the core. The overall shape is generally round. No distinct spiral arms or bar structures are discernible. There is no evidence of any major ongoing mergers or tidal disturbances, with a mostly undisturbed appearance. The light profile suggests a fairly homogenous stellar population, skewed towards older stars which would explain the orange/yellow hue. The small angular size likely indicates a considerable distance. It appears to be a relatively massive galaxy that is no longer actively forming many new stars.
