The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. It exhibits a somewhat elliptical morphology, trending towards a more rounded shape, with no apparent strong bar or spiral arm features. The core region is significantly brighter, displaying a yellowish hue, suggesting an older stellar population. The outer regions show a slightly bluer color gradient, possibly indicating more recent or ongoing star formation activity in those areas, though at a low rate. No signs of major mergers or tidal disturbances are immediately visible. The overall structure implies a galaxy that is either an elliptical galaxy or a relatively undisturbed disk galaxy seen at an oblique angle.
