The galaxy presents as a largely featureless elliptical or lenticular structure. The central region exhibits a bright, concentrated luminosity, which gradually diminishes towards the outer edges. The light profile appears relatively smooth, lacking prominent spiral arms, dust lanes, or significant knots of star formation. There's a slight elongation, but the galaxy is largely rounded in shape. The color gradient transitions from a yellowish core to a slightly bluer halo, suggesting a stellar population that is generally older in the central regions, with potentially some younger stars in the outskirts. No obvious signs of ongoing mergers or major disturbances are visible in this image, though minor asymmetries cannot be entirely ruled out with the given resolution. Overall, this galaxy seems to be relatively quiescent with a lower star formation rate.
