The galaxy presents as a relatively smooth, elliptical-like structure. Its color gradient transitions from a concentrated, reddish-orange hue at its core, suggesting an older stellar population. The overall shape appears largely spheroidal, with minimal indication of spiral arms or a distinct disk. Fainter, diffuse blue regions are observed in the outer halo, which may denote more recent star formation or scattering. There is no apparent significant interaction or merging event happening, with the galaxy appearing undisturbed, and having a round shape. The absence of intricate substructure may be indicative of an evolved stellar population.
