This galaxy presents a generally smooth, elliptical morphology, although subtle features are present. The galaxy displays a distinct prolate shape, appearing significantly elongated, almost cigar-like. The light is concentrated towards the central region with a gradual decrease towards the edges. Coloration suggests a dominant population of older stars, particularly in the central bulge, exhibiting a yellowish hue. There is faint evidence of bluer regions, potentially indicative of younger stellar populations, possibly within a nascent disk-like structure. No strong spiral arms are visible, but a hint of disk structure can be observed. There is no current significant merging activity.
