The galaxy presents a primarily bluish-white hue. The central region exhibits a concentrated, yellowish-white glow, indicative of a bulge possibly dominated by an older stellar population. Fainter spiral arm structures are suggested within the disk, although not sharply defined. The galaxy's shape appears to be elliptical, with a moderate inclination relative to our line of sight. The galaxy's outer regions gradually fade into the background, showing no sharp boundaries. A minor distortion or asymmetry can be observed in one of the outer arms, which could be from gravitational interactions.