The galaxy presents as a single, largely featureless object. It exhibits an overall elliptical morphology, appearing somewhat rounded in shape. The light profile is centrally concentrated, with a gradual decrease in intensity towards the outer edges. A slight yellow-orange hue is observed throughout the galaxy, which could be indicative of an older stellar population. No distinct spiral arms, bars, or dust lanes are readily apparent. There does not seem to be any major merging activity or disturbances. Overall, the galaxy appears to be a relatively quiescent, evolved system.
