This galaxy appears to be an elliptical galaxy, as it exhibits a generally smooth, rounded morphology with no discernible spiral arms or prominent disk structure. It is relatively compact, with a concentrated central region that suggests a high stellar density. There is a slight elongation in its shape, hinting at a possible triaxial structure. The color profile indicates a dominance of older stellar populations, evidenced by the reddish-yellow hue, although a very faint blue tinge is visible in the surrounding halo, suggesting a small population of younger, hotter stars or possible recent star formation in the outer regions. There does not appear to be any indication of a recent major merger event or significant tidal disturbance. Overall, the galaxy presents as a relatively evolved, quiescent system.
