The observed galaxy presents as a relatively compact object with a primary light distribution concentrated towards the central region. The overall color profile is dominated by shorter wavelengths, exhibiting a distinctly blue hue in the center. This is surrounded by an irregular halo showing redder and less luminous portions. The morphology suggests some level of disturbance or interaction, as it appears to deviate slightly from a purely elliptical or smooth profile, although no spiral arm structure is clearly visible. There is some evidence of asymmetry in the outer regions.
