The galaxy presents as a primarily smooth structure with a centrally concentrated bulge. The bulge region exhibits a yellowish hue, suggesting an older stellar population. Extending outward from the bulge is a disk component, showing a faint bluish tint, possibly indicating the presence of younger stars or ongoing star formation. The disk appears relatively undisturbed, with no prominent spiral arm structure or significant dust lanes visible in this image. The overall shape is somewhat elongated, leaning towards an elliptical or lenticular morphology, but with a discernible disk component. There might be a very slight indication of tidal disturbance, but the primary features suggest a well-formed, relatively quiescent system.
