The galaxy presents a largely smooth and rounded morphology. A bright central bulge dominates the structure, displaying a yellowish-orange hue, suggestive of an older stellar population. The light appears to diminish gradually towards the outer edges of the galaxy. There is a very faint hint of a disk. There is no evidence of prominent spiral arms. I observe very mild disturbance of the structure. There is no evidence of a major merger event based on visual inspection. The galaxy is considered to be relatively massive, though with a relatively low star-formation rate.
