The galaxy presents as a centrally concentrated, elliptical-shaped system. The color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated in the central bulge region. The galaxy lacks any distinct spiral arm features or prominent dust lanes, indicating a smoother morphology. Its elongated shape implies a possible classification as an elliptical galaxy of type E4 to E6, where E0 is perfectly circular, and E7 is the most elongated. There is no apparent evidence of ongoing major mergers or tidal disturbances. The overall appearance suggests a relatively quiescent, evolved galaxy with limited ongoing star formation.
