The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated bulge that appears largely featureless, with a high degree of symmetry about its major axis. The overall shape deviates slightly from perfectly circular, presenting an intermediate ellipticity. Faint, diffuse disk-like features are observed surrounding the bulge. There's no strong evidence of prominent spiral arms, bars, or other distinct morphological features. The galaxy's color profile suggests a higher concentration of older stellar populations and limited active star formation, although some bluer light is apparent in the outer regions. There are no signs of ongoing major merger activity or strong tidal disturbances, suggesting a system that is relatively undisturbed. Subtle irregularities may indicate minor past interactions.
