The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is elliptical or spheroidal, exhibiting a high degree of roundness, with only a slight deviation towards an elongated form. There is a discernible color gradient, with the central region displaying a yellowish-orange hue, indicative of an older stellar population. The outer regions transition to a bluer color. No distinct spiral arms or bar structures are visible. There are no signs of recent mergers, tidal tails, or other major disturbances. The galaxy presents a well-defined, cohesive structure.
