The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. There is a noticeable color gradient, with the central region appearing more yellowish-white, indicative of an older stellar population. Moving outward from the core, the light becomes subtly redder, possibly due to a lower metallicity or a change in the dominant stellar population. There is little evidence of spiral arms or active star formation regions. The galaxy's shape appears relatively round, displaying a degree of ellipticity but not a pronounced elongated structure. There are no signs of significant tidal disturbances or interactions with neighboring galaxies. The lack of dust lanes or prominent features suggests a well-mixed and relatively quiescent system.
