The galaxy appears as a moderately sized, somewhat diffuse object. There is evidence of both smooth and less smooth regions. A significant portion of the light is concentrated in a central region, suggesting a possible bulge. However, this is not perfectly spherical. Fainter, irregular extensions or possibly distorted spiral arms are visible, hinting at a disturbance or past interaction. The galaxy's colour appears generally redder than the surrounding objects. The overall structure suggests a transitional stage, possibly between a disk galaxy and an elliptical galaxy, or a galaxy undergoing a minor merger event. The asymmetry in the extended features indicates it may have experienced some form of gravitational interaction. Further spectral analysis is required to confirm the exact morphological type and the cause of the observed irregularities.
