This galaxy presents as a spiral type, viewed at a high inclination. It has a bright, concentrated central bulge surrounded by a flattened disk. The disk exhibits prominent spiral arms, tightly wound and somewhat fragmented. There is a suggestion of a bar-like structure, but it is not overly prominent. The bulge appears to be of moderate size, and the spiral arms are well-defined, showing some evidence of recent star formation. No major disturbances or signs of merging are observed in this image, indicating it is a relatively isolated galaxy.
