The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge is evident, exhibiting a bright, almost stellar-like core. Moving outward from the core, the luminosity gradually decreases, suggesting a smooth distribution of stars. There is very little evidence of spiral arm structures or significant dust lanes. The galaxy appears to be mostly rounded, showing no obvious signs of tidal disturbances or ongoing major mergers. The colour profile indicates older stellar populations. Faint hints of bluer light may denote recent star formation, but it appears relatively subdued across the galaxy.
