The galaxy appears to be an elliptical morphology. The light profile indicates a relatively smooth distribution, with a central concentration that becomes more diffuse towards the outer regions. The galaxy's shape is somewhat elongated, but not strongly so. The color index suggests a slightly redder core region, potentially indicating an older stellar population in the center, which transitions to slightly bluer hues in the surrounding halo, suggestive of ongoing or recent star formation. There is no indication of any major mergers or significant tidal disturbances. The object seems to be relatively isolated, displaying no obvious signs of interaction with other galaxies.
