The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical. There is little to no evidence of distinct spiral arms or a well-defined disk structure. The galaxy displays a color gradient, with the central region appearing more yellow, suggestive of an older stellar population, and the outer regions exhibiting a slightly redder hue. There is no visible evidence of active star formation regions or dust lanes. The overall appearance indicates a galaxy that is relatively evolved, likely undergoing passive evolution with a low star formation rate. There is no obvious sign of tidal disturbances or ongoing mergers, implying it is a relatively isolated system.
