The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. The overall color profile suggests an older stellar population, indicated by the yellowish hue dominant throughout the galaxy. There are no readily apparent spiral arms or dust lanes visible in this image, suggesting a lack of significant recent star formation. The galaxy’s shape is generally round, with minimal elongation or distortion, indicating it is relatively undisturbed. There is no visual evidence of ongoing mergers or tidal interactions with neighboring galaxies within the observed field. Overall, the galaxy appears to be a well-defined, evolved elliptical galaxy.
