The galaxy presents as a relatively smooth, elliptical-like object. Its morphology is dominated by a central bulge that exhibits a yellowish hue, suggesting a population of older stars. The overall shape appears somewhat elongated but not significantly cigar-shaped. There are no prominent spiral arms or distinct dust lanes visible. Faint indications of a possible minor disturbance in its structure are present, though a major merger event is unlikely based on the lack of significant disruption. The outer regions fade gradually into the background, with no pronounced halo or tidal features observed. The estimated size of the galaxy is around 5 kpc. Based on the light detected from this galaxy, it is likely still forming stars. 
