The galaxy presents as a relatively smooth, disk-like structure, elongated along its major axis. A bright central bulge region is apparent, with a yellowish-white hue, suggesting a population of older stars. The disk exhibits a bluer color profile compared to the central bulge, likely indicating ongoing star formation within the galactic plane. There appears to be a subtle disturbance, possibly indicative of a minor gravitational interaction or recent accretion event. The galaxy's overall morphology leans towards a more intermediate shape, neither perfectly spherical nor highly elongated.
