The galaxy presents as an elliptical type, exhibiting a smooth, mostly featureless structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity moving outward from the core. There is a slight elongation. The color is generally consistent across the galaxy, with a yellow-red hue indicative of an older stellar population, consistent with a low rate of star formation. There are no apparent signs of spiral arms or ongoing major mergers, though there might be a slight disturbance, such as a faint tidal tail or asymmetries.
