The galaxy presents an overall smooth morphology, with a slightly elongated profile. The central region exhibits a higher surface brightness than the surrounding areas, indicative of a concentrated galactic nucleus or bulge. The color appears to be primarily blue-green, possibly suggesting a population of younger, hotter stars or enhanced star formation activity. A faint, diffuse extension is visible on one side, hinting at a possible tidal interaction or minor disturbance. There is no strong evidence of spiral arms or a distinct disk structure.
