The galaxy presents as a relatively smooth, disk-like structure with a noticeable central bulge. The color distribution suggests a gradient, with a yellowish-white hue dominating the bulge region, potentially indicating an older stellar population. The outer disk exhibits bluer tones, possibly indicative of more recent star formation. The shape of the galaxy appears moderately elongated. There is no clear evidence of strong spiral arm structure or prominent dust lanes. There are no obvious signs of tidal disturbances or interaction with other galaxies.
