The galaxy presents as a slightly elongated, elliptical morphology. The color gradient transitions from a concentrated, bright yellow-orange core to a fainter, less defined halo of a greenish-yellow hue. The overall light distribution appears smooth, with minimal evidence of distinct spiral arm structures or prominent dust lanes. The ellipticity suggests a system that is not perfectly spherical, and may possess some degree of rotational support. The lack of strong blue emission indicates a relatively low rate of ongoing star formation. It is potentially an older, more evolved system dominated by an older stellar population. There may be the hint of a minor interaction or disturbance on one side of the galaxy.
