The galaxy presents as a smooth, elliptical morphology with a noticeable elongation. Its light profile is relatively even, suggesting a lack of prominent spiral arms or distinct features. There is a slight color gradient, appearing bluer towards the center, which may indicate a concentration of younger stars in the nuclear region. However, the overall color is redder, implying an older stellar population is dominant. The galaxy appears relatively isolated, with no immediate signs of major tidal disturbances or ongoing mergers. It exhibits a generally regular shape, deviating minimally from a perfect ellipse.
