The galaxy presents as a relatively smooth, centrally concentrated object with a near-elliptical morphology. There is a clear central bulge region exhibiting a yellowish hue, suggesting a population of older stars. Surrounding the bulge, a faint, diffuse disk or halo is observed, exhibiting a slightly bluer color, possibly indicating younger stellar populations and ongoing star formation. The overall structure appears undisturbed, lacking any prominent tidal features or indications of a recent major merger event, although there is some hint of a slight disturbance in the evenness of the halo. The galaxy's shape is more in between round and cigar shaped. No prominent dust lanes or spiral arm structures are readily apparent in the image. The light is generally evenly distributed, indicating a relatively stable system.
