The galaxy presents a moderately bright, centrally concentrated luminosity profile. There is evidence of significant morphological disturbance. The central region is relatively smooth and bright, suggesting a possible bulge. However, the outer regions exhibit irregular structures and hints of tidal features, potentially indicating a past or ongoing interaction/merger event. The overall color profile suggests a mixture of stellar populations, with a central blue-white core possibly indicating the presence of younger stars, surrounded by a more yellowish-red halo of older stars. The outer structures are faint and diffuse, extending away from the main body.
