The galaxy presents as a somewhat elliptical, centrally concentrated structure. Its light profile appears smooth, with a gradual decline in surface brightness from the core outwards. The core exhibits a yellowish hue, suggesting an older stellar population. Progressing outwards, the color shifts toward redder tones in the fainter outer regions. No prominent spiral arms, bars, or dust lanes are apparent in this image. There are no indications of any major ongoing mergers or tidal distortions. A potential small disturbance or artifact is present on the lower right, but the classification is not definitive. 