The galaxy appears as a single, centrally concentrated object with a generally smooth and rounded morphology. There is no clear evidence of spiral arms, a prominent disk structure, or significant tidal features indicative of recent major mergers. The color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue, particularly in the central regions. There is a subtle color gradient, with the core appearing slightly more yellow than the outer regions, which are closer to red. No significant dust lanes or active star-forming regions are discernible in this image. The overall form is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy viewed at a considerable distance. The object exhibits no visible signs of significant disturbance or ongoing mergers.
