The galaxy presents as a single, dominant object with a relatively smooth, spheroidal morphology. It exhibits a concentrated, round light profile, showing minimal evidence of spiral arm structures or significant dust lanes. There may be a slight asymmetry that is barely visible, but the general morphology is generally smooth. The galaxy displays a color gradient across its surface, with a slightly more red/orange core gradually fading into a yellow/white halo region. There is no obvious evidence of any major or minor merger events in the recent past, and the galaxy appears to be relatively undisturbed.

Based on the galaxy's apparent size, smoothness, and estimated distance, this galaxy is likely a lenticular or elliptical galaxy. The estimated star formation rate appears to be fairly low, potentially indicating that the galaxy has largely exhausted its supply of gas and dust for forming new stars.
