The galaxy presents a complex morphology. The central region exhibits a bright, relatively smooth structure, possibly a bulge. Surrounding this is a fainter, more diffuse halo. There are faint structures to the side, likely caused by distortions. The color gradient suggests some level of ongoing star formation. The galaxy may be undergoing tidal disruption or a minor merger event. The observed irregularities in its morphology suggest the influence of external gravitational interactions, potentially with another galaxy. Further spectroscopic analysis is needed to confirm the nature of these interactions and to determine the galaxy's redshift and internal kinematics.
