The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central region. The overall color appears to be slightly redder compared to typical spiral galaxies, suggesting a population dominated by older stars. There is a lack of discernible spiral arms or prominent dust lanes. However, there may be some minor disturbances or irregularities in its shape, indicating potential interactions with nearby galaxies or past merger events. The galaxy does not appear perfectly spherical, showing some degree of elongation.
