The galaxy appears to be relatively compact, displaying a slightly elongated morphology along a roughly horizontal axis. The central region exhibits a brighter, more concentrated luminosity profile, surrounded by a fainter, more diffuse halo. There may be subtle irregularities or features suggesting a possible ongoing interaction, disturbance, or merging event. The primary color is a slightly blue-green hue, which could indicate the presence of younger stellar populations. However, the overall color is relatively uniform across the galaxy's extent. There is no definitive spiral structure evident.
