The galaxy presents as a relatively smooth, elliptical-like structure. It appears mostly homogenous in color and luminosity, with a concentrated central bulge. The primary hue is a yellow-orange, suggesting an older stellar population. There is a subtle indication of a very faint and diffuse disk-like component extending beyond the central region. The lack of defined spiral arms or significant dust lanes supports a classification leaning toward early-type morphologies. The object shows no obvious signs of tidal disturbances or ongoing major merging events.
