The galaxy presents as a slightly elliptical, disk-like structure, exhibiting a central bulge region with a high degree of smoothness. The disk component shows some subtle features, though they are not sharply defined. The color profile indicates a possible active star formation, with a blue hue becoming slightly more pronounced toward the central region and some minor areas within the disk. Faint hints of tidal disturbances are visible, suggesting a potential recent interaction or merger event. The galaxy appears relatively isolated, with no immediate nearby galaxies that could be causing major gravitational disruption. The galaxy’s overall morphology suggests it may be undergoing a transition from a more active, star-forming state to one that is more quiescent.
