The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There is no apparent disk structure or spiral arms. The color profile is generally uniform across the galaxy, exhibiting a slightly yellowish hue, which suggests a population of older stars. There is no evidence of significant dust lanes or patches of active star formation within the galaxy. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or merging events with neighboring galaxies. The overall impression is that of a well-established, passively evolving elliptical galaxy.
