The galaxy presents as a luminous, elongated structure, likely a flattened elliptical or a lenticular galaxy seen at an oblique angle. The central region exhibits a higher concentration of light, appearing yellow-orange in color, suggestive of an older stellar population with fewer active star-forming regions and an abundance of evolved stars. Moving outwards from the core, the luminosity decreases, and the color shifts towards a slightly bluer hue, hinting at the presence of some younger stars in the galactic disk or outer regions, though not particularly prominent. The overall form shows a smooth distribution of light, with no obvious spiral arm structures or significant dust lanes visible. The axial ratio suggests a considerable degree of flattening, and the lack of strong tidal features indicates no recent major mergers. The morphology appears relatively undisturbed, indicative of a galaxy that has largely settled into a stable, quiescent state. There is a small chance of a minor interaction, but the galaxy itself appears largely undisturbed.
