The galaxy presents as a centrally concentrated object with a largely smooth morphology. The light distribution appears relatively even, with no prominent spiral arm structures or a well-defined disk. The galaxy's shape is approximately elliptical, exhibiting some deviation from a perfect circle. There is no evidence of a major merger, and the system appears relatively undisturbed. The galaxy exhibits a redder color, suggesting an older stellar population and/or significant dust content. This red color is more consistent with the "red sequence" of galaxies dominated by older stars and lower star formation rates, though it does not appear to be perfectly on the red sequence given it is a "goldilocks galaxy".
