The galaxy presents a generally smooth appearance with a centrally concentrated bulge exhibiting a yellowish hue, indicative of an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component. There's evidence of bluer star formation regions within the disk, particularly in the area adjacent to the bulge. The overall shape of the galaxy is close to round. There might be a slight tidal distortion or asymmetry observable in the fainter outer regions of the disk, but the galaxy doesn't appear to be undergoing a major merger, though minor disturbances cannot be ruled out.
