The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. A bright central region dominates, suggesting the presence of a significant galactic nucleus. A fainter, diffuse halo surrounds the bright core, gradually fading into the background. The overall shape is somewhat elliptical, with deviations suggesting a possible interaction or internal disturbance. There is evidence of a slight asymmetry in the halo's distribution of light. The color of the central region is relatively blue, suggesting a young stellar population. Overall the galaxy appears relatively compact.
