The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The light distribution appears to be dominated by an older stellar population, indicated by the yellowish-white hue of the galaxy's core. A distinct lack of resolved spiral arms or dust lanes is evident. There is little indication of ongoing or recent star formation based on the color profile. The galaxy appears isolated, with no obvious signs of tidal disturbances or interacting companions nearby. Overall, it seems to be a well-formed, evolved galaxy that is likely a lenticular galaxy, or an elliptical galaxy.
