The galaxy presents as a relatively smooth, rounded structure, suggestive of an elliptical morphology or a lenticular galaxy viewed face-on. The light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The primary color is a yellow-orange hue, possibly indicating an older stellar population and a lower rate of ongoing star formation. There is a faint bluish structure that may be a tidal stream or the remnant of a merger. No distinct spiral arms or prominent dust lanes are visible. The galaxy seems to be fairly isolated with only minor disturbances present.
