The galaxy presents as a roughly elliptical, moderately luminous structure with a concentrated central bulge. The core exhibits a yellowish-white hue, suggesting a population of older stars. Extending outward from the core is a fainter, diffuse halo with a hint of bluish tint. The overall morphology suggests a system with a relatively smooth profile, though subtle irregularities are discernible. There are faint indications of disk-like structures, though they are not clearly defined. There is a slight asymmetry to the galaxy. The image suggests the possibility of minor disturbances or interactions, as it shows a slightly asymmetrical shape which could be evidence of past or ongoing merger events.&#x20;
