The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge that exhibits a yellowish hue, possibly indicative of an older stellar population. The overall shape is somewhat elongated, leaning toward a cigar-like form, but largely presents as in between round and elongated. There is a subtle gradient in color, with the core region appearing brighter and more golden compared to the outer regions, which appear more diffuse with a slight blueish tinge. There are no visible signs of active merging or major disturbances within the immediate vicinity of the galaxy; rather, the morphology suggests it is a relatively isolated system with a stable configuration. There may be very minor disturbances, but they do not strongly effect the overall appearance.
