The galaxy presents a generally smooth morphology, appearing largely featureless with minimal evidence of a disk-like structure. The light distribution suggests a spheroidal shape, leaning toward a circular form rather than a highly elongated or cigar-like appearance. There is no strong indication of ongoing major mergers or significant tidal disturbances; the structure seems relatively relaxed and undisturbed. The color profile exhibits a redder hue in the central region, shifting towards slightly bluer tones in the outer parts. This color gradient could indicate a difference in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars in the outskirts, hinting at possible ongoing, though weak, star formation activity.