The galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular classification. It presents a centrally concentrated brightness profile, fading gradually towards the edges. The galaxy appears largely featureless, lacking prominent spiral arms or dust lanes. There is a slight elongation visible in the galaxy's shape, indicating it is not perfectly spherical, with the appearance of being "in between" round and cigar shaped. There may be evidence of a very minor disturbance to the structure of this galaxy. The color indices suggest the galaxy is composed of an older stellar population. Star formation rates appear to be generally low.
