The galaxy presents a smooth, elliptical morphology. Its color profile suggests an older stellar population, with a yellow-red hue concentrated towards the galactic center. A slight elongation is observed along its major axis, giving it a somewhat cigar-shaped appearance. There's no discernible evidence of spiral arm structure or active star formation regions from this image alone. No major mergers appear to be occurring. Minor asymmetry or disturbances cannot be ruled out entirely, but are not readily apparent. The galaxy appears relatively isolated within its immediate vicinity.
