The galaxy presents as a centrally concentrated object, appearing smooth in overall texture, although its features are somewhat unresolved. It exhibits a prolate spheroid morphology, appearing elongated, with a cigar-shaped structure. The core region appears brighter and more intensely luminous in comparison to the outer regions. Color gradients are observed, with a yellowish-orange hue concentrated towards the central bulge, indicative of an older stellar population, while bluer tints are subtly present towards the periphery, potentially signifying the presence of younger stars or regions of ongoing star formation. There is no apparent dust lane or spiral arm structure discernable at this resolution. Some minor disturbances may be present in the shape of the galaxy, indicating a history of interactions with other galaxies. Overall, it appears as a relatively undisturbed, moderately massive galaxy with likely moderate star formation activity.
