The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated with a high degree of roundness. A slight elongation is observed, but the overall shape is more akin to a spheroidal structure than a flattened disk. There is no immediately apparent evidence of spiral arm structure or significant dust lanes. The central bulge region dominates the galaxy's light profile, displaying a bright, concentrated luminosity. The color indices suggest a relatively evolved stellar population, with a redder hue indicative of older stars, possibly indicating a diminished rate of active star formation, which corresponds to a low specific star formation rate (SSFR). There is no obvious ongoing major merger activity or strong tidal disturbances affecting the galaxy's overall structure; it shows a quiescent state. The size, as estimated by half-light radius, is consistent with a galaxy of moderate size. The color gradient within the galaxy indicates the central regions are relatively redder than the outer regions, perhaps due to differences in stellar populations or dust content.
