The galaxy presents a generally smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, unresolved core that appears roughly circular. The color profile shows a gradient from a relatively bluer center to redder outer regions. There is little to no evidence of spiral arms or a distinct disk structure; instead, the light distribution fades gradually outward from the core in a spheroidal fashion. No major disturbances are visible. Based on the color, it is likely that there is little dust content in the galaxy. It shows a lack of prominent features or asymmetries. The outer edges are somewhat irregular.