The galaxy presents as an elliptical or lenticular-like morphology, exhibiting a smooth, concentrated central bulge that dominates the overall structure. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. Faint and indistinct features may be embedded in the disk, but this cannot be said with certainty based on the image. The galaxy appears to be moderately massive and does not currently show signs of significant star formation activity. There is no apparent indication of tidal disturbances, major mergers, or strong interactions with neighboring galaxies, and the disk appears to be stable.
