The galaxy appears to be a spiral type, though potentially viewed at a high inclination. A central bulge is present, exhibiting a bright, condensed morphology. Surrounding the bulge, faint, diffuse arm structures are visible. These arms exhibit subtle color variations. There are hints of minor disturbances in the galaxy's morphology, potentially indicative of a past or ongoing minor merger event. Overall, the galaxy exhibits a complex morphology. Further spectroscopic analysis is recommended to confirm the classification and investigate the potential merger activity.
