The galaxy presents as an elliptical morphology, appearing generally smooth and centrally concentrated with no readily discernible spiral arms or bar structure. There is a gradual decrease in luminosity from the core outwards. It exhibits a yellowish to red hue which possibly indicates an older stellar population. The object presents as moderately compact. There does not appear to be any evidence of major mergers or tidal disturbances. There appears to be minimal star formation, consistent with a population dominated by older stars. The shape tends toward round rather than elongated.
