The galaxy presents as an elongated, cigar-shaped structure. The central bulge exhibits a relatively smooth, diffuse appearance, transitioning outward to a less defined disk. Coloration suggests a mix of stellar populations. The core region appears to be composed of older stars, exhibiting a yellowish-white hue. The outer edges are somewhat bluer, implying the presence of younger, hotter stars and possible star forming regions. There is a noticeable, localized region of enhanced red coloration, indicating areas of dust obscuration or a distinct population of older stars. Overall, there is no evidence of spiral arm structure or active galactic nucleus activity.
