The galaxy presents as a spiral type, exhibiting a prominent, moderately bright central bulge that appears somewhat elongated. The disk structure is clearly visible, with well-defined spiral arms extending from the central region. The arms appear relatively loosely wound. There is a possible bar-like structure that crosses the central bulge. In terms of color, the central bulge displays a yellowish hue, suggesting a population of older stars. The spiral arms exhibit bluer tones, indicating regions of active star formation. There are some irregularities or disturbances in the galaxy's morphology, indicative of possible gravitational interactions or a recent merger event. Overall, the galaxy displays a complex morphology.
