The galaxy presents a generally smooth and rounded morphology. The central region displays a concentrated, bright core, suggesting a substantial stellar population. The color profile is consistent with an evolved stellar population, with a yellow-orange hue dominating the galaxy's overall appearance. Faint, diffuse extensions surround the core, gradually fading into the background. There is no clear evidence of spiral arms or a prominent disk structure, indicating it is likely an elliptical galaxy. There are no strong indications of active star formation, although there is faint blue light present in the diffuse edges of the galaxy. There is no clear evidence of ongoing or recent merger activity based on the symmetry and lack of tidal tails or other major disturbances.
