The galaxy presents as a generally smooth, elliptical structure. It exhibits a moderately elongated, cigar-like morphology. A central bulge region is visible, appearing somewhat brighter and more concentrated than the surrounding disk. The color profile suggests a redder core transitioning to a slightly bluer outer region, which may indicate differing stellar populations or dust content between the core and disk. No obvious spiral arm structures or significant disturbances are apparent, although subtle irregularities may be present upon closer inspection. There is no evidence of active merging or major tidal disruption.
