The galaxy presents a largely smooth morphology with a slight elongation, appearing as a flattened spheroid, with a suggestion toward a cigar shape, but not extremely so. The central region exhibits a higher surface brightness, indicating a prominent galactic nucleus. Overall, the color appears largely consistent, with a subtle blue hue across the disk, suggestive of active star formation. There are possibly some minor disturbances in the outer regions, but they are fairly faint. No clear spiral arm structure is discernible. The disk is moderately inclined relative to our line of sight, and the galaxy appears to be relatively isolated, showing no signs of major mergers or interactions with other galaxies.
