The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light profile. It presents a morphology that is more rounded than elongated, suggesting a low degree of intrinsic flattening. The galaxy's color index suggests a redder overall color, indicative of an older stellar population and a relatively low current star formation rate. No significant tidal features or morphological disturbances are readily apparent, suggesting that the galaxy is likely in a relaxed state and not currently undergoing major interactions or mergers. While it seems to not be undergoing a major disturbance, it is not impossible that a minor interaction is taking place.
