The galaxy presents as a relatively smooth, elliptical morphology. Its light distribution appears concentrated towards the center, exhibiting a bright, moderately resolved core. There is a subtle color gradient observed, with the central region presenting a more yellow-orange hue, suggestive of an older stellar population. Fainter, slightly bluer light surrounds the central region, potentially indicating the presence of some younger stars or regions of ongoing star formation, though this feature is subdued. The galaxy is moderately elongated, appearing between round and cigar shaped, with no distinct spiral arm structures visible at this resolution. There's no obvious evidence of a major ongoing merger or tidal disturbances, though minor irregularities or disturbances cannot be ruled out based on the image alone. The overall impression is that of a galaxy dominated by an older stellar population, with a low to moderate amount of recent star formation activity.
