The galaxy presents as a somewhat elongated, luminous object with a smooth appearance. The central region exhibits a concentrated glow, appearing more yellow or golden in color. This suggests a higher density of older stars. Moving outwards from the center, the luminosity decreases, and the color shifts towards a slightly bluer hue, implying a younger stellar population within the galactic disk. There are no distinct spiral arm structures visible, and the overall morphology suggests a disk-like structure, possibly a lenticular galaxy or a spiral galaxy seen at a significant angle. There is a faint outer halo region, but there is no evidence of significant tidal disturbances or interactions.