The galaxy presents as a lenticular or edge-on spiral morphology, displaying a smooth, elongated profile. The major axis of the galaxy is significantly longer than the minor axis, suggesting a flattened disk structure. There is no discernible bulge component, or it is very small, and no apparent spiral arm structure. The color appears to be relatively uniform across the galaxy, with a slightly redder hue, indicating a population of older stars and/or a significant amount of dust obscuring any younger, bluer stars. The overall appearance indicates a galaxy with suppressed star formation activity. There is no evidence of any significant interaction with neighboring galaxies, such as tidal tails or distortions.
