This galaxy exhibits a generally smooth morphology, with a slightly elongated shape, appearing neither perfectly round nor highly flattened. There is a noticeable concentration of light towards the center, suggesting a substantial bulge component. The color appears to be predominantly yellow-orange, indicative of an older stellar population. There is no strong evidence of spiral arms, bars, or major disturbances due to mergers. Minor irregularities or disturbances appear to be present in the outer regions of the disk.
