The galaxy presents as a central bulge-dominated system, exhibiting a smooth, elliptical morphology. The primary light emission appears yellowish-orange, likely indicative of an older stellar population. There are faint hints of a flattened disk surrounding the bulge, but it lacks defined spiral arms or prominent dust lanes. The overall shape is largely spheroidal, although it deviates slightly from a perfectly circular form, showing more of an in-between shape. There are no apparent signs of significant tidal disturbances, major mergers, or strong interactions with neighboring galaxies. A very slight bluish tinge is observed on its outer edges which indicates some possible star formation.
