The galaxy presents as a single, luminous object, exhibiting a generally smooth morphology. Its shape appears to be somewhat elliptical, tending toward a disk-like structure but without any prominent spiral arms or bar features immediately visible. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a substantial galactic nucleus. Fainter halos extend outwards. A slight color variation is observed within the galaxy, transitioning from a yellowish hue in the core to a subtly bluer tint in the outer regions. This suggests a possible difference in the stellar population, with older stars concentrated in the center and younger stars potentially populating the outskirts. There may be a very minor disturbance in the structure of the galaxy. This galaxy appears to be in the distance.
