The galaxy appears to be a relatively smooth, elliptical system. Its overall shape is oblong, with a higher concentration of light towards the center, indicating a prominent bulge. The color profile suggests an older stellar population, with the core exhibiting a yellowish-white hue. There's little evidence of spiral arm structure or significant dust lanes. Faint bluish edges surround the central bulge, hinting at possible recent, but limited, star formation activity in the outer regions. The galaxy's morphology appears undisturbed, with no clear signs of ongoing or recent major merger events. Minor asymmetry might suggest minor interaction, but further investigation is required.
