The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The core region exhibits a pronounced concentration of light, appearing almost unresolved at this resolution, suggestive of a bulge-dominated system. 

Moving outward from the core, the galaxy appears to fade smoothly into the background sky. There is some irregularity in the outer isophotes and subtle color variation, indicating possible weak features or faint spiral arms. These features lack a clearly defined structure. The color gradient across the galaxy implies a moderate population of young stars, especially in the outer regions. There is no evidence of significant tidal disturbances or a recent major merger event.
