The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge that gradually fades toward the edges. The overall color is yellowish, suggesting a population of older stars. There is a hint of redder tones in a few regions around the core, which may indicate areas of dust obscuration or the presence of some older, cooler stars. The galaxy's light distribution appears quite uniform without significant spiral arm features or prominent star-forming regions visible. The object has a moderately compact size, the shape being somewhat rounded rather than elongated. There is no obvious evidence of tidal tails or significant distortions indicative of a recent major merger event, though there may be some very subtle signs of minor disturbances within the outer regions of the galaxy.
