The galaxy appears as a small, elongated structure, exhibiting a smooth, lenticular morphology. The overall color is whitish-blue, indicative of a stellar population with intermediate-aged stars. The light distribution is relatively uniform, lacking prominent spiral arms or distinct features. There is no apparent central bulge or nucleus, further supporting a classification towards the smooth end of the morphological spectrum. The galaxy's orientation is nearly edge-on, making it difficult to discern any internal structure or potential dust lanes. No signs of ongoing major mergers or tidal disturbances are observed, although subtle irregularities in the light distribution might indicate minor interactions in its past. The compact size and high degree of smoothness suggest that star formation may be suppressed relative to other galaxies with similar mass.
