The galaxy presents a largely smooth, elliptical morphology. Its color profile appears generally redder, with a concentration of light toward the central bulge. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy's overall structure seems well-defined, with a gradual decline in luminosity from the center outwards. No obvious signs of ongoing major merging events or significant tidal disturbances are apparent, although some minor irregularities in its outer regions cannot be ruled out. Given the observed characteristics, the galaxy is likely a relatively massive system with a low star formation rate.
