The galaxy presents as an elliptical-like morphology, exhibiting a smooth and generally featureless structure. The light distribution appears centrally concentrated with a gradual decline in intensity towards the outer regions. It has a mostly rounded shape, with an intermediate appearance between circular and elongated.  There is little evidence of spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing a major merger or significant tidal disruption. The color indices suggest that the galaxy is redder in the central region, possibly indicating an older stellar population, while the bluer light on the outskirts suggests that the outer regions have younger star forming regions.
