The galaxy presents as an ellipsoidal object with a somewhat elongated morphology. There is a distinct central bulge exhibiting a yellowish-orange hue, potentially indicating an older stellar population. A fainter, bluer disk component is suggested by the subtle color gradient extending outwards from the core. The overall structure appears relatively smooth, with only minor hints of irregularities or disturbances. A small, reddish point source is visible near the outer edge of the disk, possibly a compact region of active star formation or a background object. The estimated size and absolute magnitude suggest this is a relatively large and luminous galaxy. Based on the colors, there is likely ongoing star formation, but at a low rate. The overall visual impression is that this is a galaxy transitioning from a spiral type towards a more elliptical morphology. There is no clear evidence of major mergers, but minor disturbances or interactions may be present.