The galaxy presents as a flattened, elongated structure, suggesting an elliptical morphology viewed at a significant angle relative to its plane. The central region exhibits a brighter, more concentrated luminosity profile, indicative of a nucleus or bulge. The color gradient across the galaxy appears relatively smooth, with a subtle shift towards redder hues in the outer regions compared to the central area. The outer edges are not well-defined, blending gradually into the background sky. There is little to no evidence of distinct spiral arms or prominent dust lanes, further supporting the classification as an elliptical or lenticular type. The overall appearance suggests a relatively evolved system with potentially reduced star formation activity. No obvious signs of tidal interactions or ongoing mergers are visible.
