The galaxy presents a flattened, elliptical morphology, appearing elongated along its major axis. It exhibits a smooth, diffuse light distribution with a bright, concentrated central region, likely a galactic bulge. Hints of spiral structure are subtle, possibly indicating a weak or tightly wound spiral arm configuration. The galaxy's color suggests a mix of stellar populations; the central bulge displays a whiter hue indicative of older stars, whereas the outer disk regions exhibit a bluer tinge, potentially suggesting ongoing star formation. There's a slight asymmetry in the light distribution of the disk which may be due to gravitational interactions or gas accretion. No major merging events are clearly visible, and while tidal features or strong disturbances are not apparent, minor perturbations might be present. Overall, the galaxy appears to be a disk galaxy, with a high fraction of old stars and a moderate amount of recent star formation.
