The galaxy presents an overall smooth morphology with a noticeable disk-like structure. The central region displays a concentrated yellowish-white hue, suggesting a significant population of older stars. Emanating outward from this core, faint extensions of a greenish-blue color are visible. These extensions suggest a presence of relatively higher star formation, possibly related to the disk structure, and hint at the presence of ionized gas. There are no apparent signs of major disturbances or ongoing mergers; the structure appears largely undisturbed. It exhibits an intermediate roundedness. The galaxy's reddish color hints at it being at a relatively large distance.
