The galaxy presents a largely smooth and rounded morphology. The light distribution is centrally concentrated, with a gradual decrease in intensity toward the outer regions. The color index suggests the presence of an older stellar population, with a yellowish-red hue dominating the galactic body. There is a subtle hint of bluer light towards the edges, suggesting the possible presence of some younger stars, but the overall impression is that of an evolved system. The galaxy exhibits minimal discernible structure; spiral arms, bars, or prominent dust lanes are not apparent in the image. There might be slight disturbances in the galaxy's structure, but nothing to suggest that it is undergoing a major merger. 
