The galaxy presents as a luminous, spatially extended object with a centrally concentrated morphology. The light distribution appears relatively smooth, with a dominant spheroidal component. There is evidence of a slight distortion in the overall shape, suggesting a possible interaction or ongoing merger event. This is further suggested by the presence of clumpy structures and disturbed features in the outskirts of the galaxy, indicating recent or ongoing tidal forces. The galaxy exhibits a color gradient, transitioning from bluer hues in the outer regions to redder tones in the core, indicative of varying stellar populations and dust content. The redder central region suggests an older stellar population, potentially with a significant amount of dust obscuration, while the bluer regions could indicate more recent star formation activity. Overall, the galaxy seems to be in a state of transition, potentially evolving through a merger-driven process.
