The galaxy presents a generally smooth appearance, with a slight elongation suggesting an intermediate shape between round and cigar-shaped. A central, somewhat brighter region is observed, possibly indicating a bulge or active galactic nucleus. There are hints of subtle features or irregularities in the disk. Overall, the galaxy does not display any obvious signs of major mergers, although minor disturbances might be present. The estimated size is on the order of a few kiloparsecs, suggesting it's likely a dwarf galaxy. The color is indicative of a redder population suggesting that star formation is suppressed.
