The galaxy presents an elongated, cigar-shaped morphology, with a smooth overall appearance. A central bulge dominates the structure, displaying a yellowish-orange hue, suggesting a population of older stars. Fainter, bluer light extends outward from the core. There is a hint of a disk-like component surrounding the bulge, although it's not clearly defined. No spiral arms or prominent dust lanes are visible. There is no evidence of any major merger events or tidal disturbances.
