The galaxy presents a generally smooth, elliptical morphology. It exhibits a central concentration of light, indicative of a prominent bulge. The color profile appears redder towards the center, suggesting an older stellar population. The outer regions show a bluer hue, hinting at the presence of younger stars or ongoing star formation, although the rate of star formation appears to be relatively low overall. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent merger events. The isophotes are generally smooth and elliptical in shape, though there is some subtle irregularity.
