The galaxy appears to be an elliptical galaxy, characterized by a smooth, relatively featureless morphology. The light profile suggests a centrally concentrated luminosity distribution, typical of elliptical galaxies. The central region exhibits a yellowish-orange hue, which likely indicates an older stellar population. The galaxy is reasonably round, but appears slightly elongated. There is no clear evidence of spiral arms or significant dust lanes within the galaxy's structure. No signs of major tidal disturbances or ongoing mergers are readily apparent. The light distribution fades gradually towards the outer edges, suggesting a smooth transition in stellar density.
