The galaxy presents as an elliptical morphology, though not perfectly spherical; it appears somewhat flattened. The central bulge is prominent and displays a significantly higher surface brightness compared to the surrounding galactic halo. The color of the bulge appears more reddish or yellowish, possibly indicative of an older stellar population. The outer regions exhibit a bluer hue, suggesting the presence of younger, hotter stars and/or ongoing star formation, albeit at a moderate rate. There are no clear signs of spiral arm structures or a distinct galactic disk. The galaxy doesn't show obvious signs of major mergers or tidal disturbances, although minor irregularities in the outer halo cannot be ruled out due to the resolution. Overall, the galaxy appears to be a fairly massive, relatively undisturbed system, somewhere in transition between a classic elliptical and a more actively star-forming disk galaxy.
