The galaxy presents a predominantly smooth, elliptical morphology with a high degree of central concentration. The color profile suggests an older stellar population, with a redder hue dominating the galaxy's overall appearance. There is little evidence of active star formation regions. The shape is nearly circular, with a slight elongation that is barely perceptible. No distinct features are visible, such as spiral arms, dust lanes, or a prominent bar structure. There is no indication of any major merger event or significant tidal disturbances. The galaxy appears isolated and undisturbed, exhibiting a classic spheroidal form typical of early-type galaxies.
