The galaxy presents as a centrally concentrated, smooth object. Its color profile is largely homogenous and leans towards the redder end of the spectrum. There is a subtle, but noticeable falloff in intensity moving from the galactic center towards its periphery, which suggests a gradual decrease in stellar density. No distinct spiral arms or bar structures are discernible. Furthermore, there is an absence of any prominent tidal features or other indications of recent major merger events. The object is generally elliptical in shape, but close to round. Based on the observed characteristics, this galaxy could likely be classified as an elliptical galaxy.
