The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a flattened, elongated shape. The central bulge appears prominent, with a smooth, diffuse light distribution suggestive of an older stellar population. There is a suggestion of a faint disk. The color profile is generally redder in the central regions, shifting toward slightly bluer hues in the outer regions. There are no clearly defined spiral arms or dust lanes visible, and the overall structure appears relatively undisturbed, showing no signs of ongoing major mergers or significant tidal interactions. Based on this information it appears to have a very low rate of star formation.
