The galaxy presents as a relatively smooth, elliptical-like structure. It has a bright, concentrated central bulge that appears yellowish-white in color, suggesting an older stellar population dominating the core. The outer regions exhibit a fainter, bluer hue compared to the core, possibly indicating the presence of younger stars or ongoing star formation, although the rate appears to be relatively low. There is a slight elongation visible, but no distinct spiral arms or bars are discernible. Faint hints of asymmetry exist, but no clear evidence of a major ongoing merger is apparent. The galaxy does not appear to be perfectly round, exhibiting a degree of flattening.
