The galaxy presents a generally elliptical morphology, appearing elongated with a relatively smooth light distribution. There is no prominent bulge or distinct spiral arm structure discernible in this image, lending it a somewhat featureless quality. The core region displays a concentrated brightness, suggesting a higher density of stars or possibly an active galactic nucleus. The overall color is slightly reddish, indicating an older stellar population with ongoing star formation at a moderate rate, suggesting that the galaxy is not entirely passive. There is no visible sign of any major merging events or tidal disturbances. The galaxy appears largely isolated.
