The galaxy appears as a slightly elliptical, diffuse object with a concentrated central bulge. The light distribution suggests a relatively smooth morphology, with no obvious spiral arm structures or prominent dust lanes visible. There is a gradual decrease in luminosity from the core to the outer regions. The galaxy presents a yellowish-white hue, indicating a stellar population that is likely dominated by older, less massive stars, with possibly ongoing, but not significant, star formation activity. There are no signs of any major tidal disturbances or ongoing mergers. The overall appearance aligns with an intermediate type between a spiral and an elliptical galaxy, possibly a lenticular galaxy, though no disk structure can be clearly discerned.