The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated bulge, indicating a high density of stars. Moving outwards, the galaxy fades gradually into a less luminous halo. The color profile suggests an older stellar population, with a general lack of blue light indicative of ongoing star formation. There appears to be a slight asymmetry in the outer regions, but overall, it's predominantly symmetrical. There isn't any clear evidence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or recent merger events.
