The galaxy presents an elliptical morphology, with a smooth and relatively featureless appearance. The central region exhibits a concentration of light, appearing bright and somewhat diffuse, suggesting a significant stellar population. The galaxy appears to be moderately red in color, particularly towards the center, indicating an older stellar population and relatively low ongoing star formation. There is little evidence of spiral arms, dust lanes, or other distinct structural features typically observed in spiral galaxies. The overall shape is generally round, with only a slight elongation. There is no clear evidence of any ongoing merger activity or significant tidal disturbances.
