The galaxy presents as a somewhat elliptical structure, appearing mostly smooth with a concentrated central bulge. The color profile suggests an older stellar population dominating the bulge, indicated by a reddish-orange hue. A disk structure is faintly discernible, exhibiting bluer colors suggestive of ongoing star formation. The overall morphology appears largely undisturbed, though subtle irregularities may be present that would require higher resolution imaging for confirmation.
