The galaxy presents a generally smooth, elliptical morphology. The overall color is slightly reddish, possibly indicative of an older stellar population and reduced star formation activity. There is evidence of a minor tidal disturbance or possible interaction with a nearby object; a slight asymmetry or faint extension in the halo region is observed. The galaxy appears relatively compact in size. A small central bulge is apparent. No prominent spiral arms or dust lanes are discernible in the available image. There are no apparent indications of a recent major merger. Overall, the galaxy is most likely an evolved system transitioning towards quiescence.
