The galaxy presents as a centrally concentrated object with a relatively smooth appearance. The core exhibits a bright, yellowish hue, suggesting an older stellar population dominating the central region. Fainter, diffuse extensions of bluer light surround the core, implying the presence of some younger stars or ongoing, though potentially limited, star formation within the outer regions of the galaxy. There is no obvious spiral structure or distinct features such as prominent dust lanes or tidal tails. The overall shape is somewhat elongated, with the central bulge appearing more rounded than the broader galactic halo. Subtle irregularities in the outer regions hint at possible minor disturbances, although no major merger events are immediately apparent.
