The galaxy presents a generally smooth, rounded morphology, suggesting an elliptical type. It appears largely devoid of prominent spiral arms or significant disk-like features. The light distribution is relatively even, with a centrally concentrated brightness that diminishes gradually toward the outer edges. The object exhibits a yellow-red color profile, indicative of an older stellar population and reduced recent star formation activity, which is typical of ellipticals. There is no obvious evidence of significant ongoing mergers or major tidal disturbances, although some minor asymmetries cannot be ruled out based on this image alone. Overall, this galaxy seems to be a fairly well-formed, relatively evolved system.
