The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The morphology is primarily elliptical, exhibiting a high degree of roundness, close to 90%. There is minimal visual evidence of spiral arms or a defined disk structure. The light distribution suggests a lack of significant dust lanes. The galaxy has an effective radius of approximately 7 kpc. The color gradient indicates a population of older stars, possibly indicative of a passive evolution stage. No prominent tidal features or signs of recent major merger activity are observed.
