The galaxy presents as a moderately bright, disk-shaped structure with a relatively smooth appearance overall. It is observed at a significant inclination to our line of sight, giving it an elongated, lenticular form. The central bulge region appears subtly reddish in color, perhaps indicating an older stellar population, while the outer disk exhibits a bluer tint, which is consistent with the presence of younger, hotter stars associated with ongoing or recent star formation. There are no obvious spiral arm structures easily discernible. The overall morphology suggests a galaxy that has not experienced a major merger event recently but does display some minor disturbances. Based on the low star formation rates inferred from the image, it is likely that the galaxy is dominated by older stars.
