The galaxy presents a primarily smooth morphology, exhibiting a notable lack of distinct spiral arms or a prominent central bar structure. The light distribution suggests a spheroidal shape, appearing largely elliptical. A bright central bulge dominates the overall appearance, fading into a more diffuse halo. The colors indicate a population of older stars, with a yellowish hue concentrated in the core region, transitioning to bluer tints in the outer regions. There is a subtle indication of possible minor disturbances, possibly caused by a small ongoing or past merger. Despite the largely smooth nature, there might be faint hints of a disk-like component when accounting for the slight blue shift in the outer regions of the galaxy. The galaxy overall has a compact, relatively rounded appearance.
