The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, appearing mostly round with a slight elongation along an indiscernible axis. The color profile suggests an aging stellar population, with a predominantly red/yellow hue in the core, transitioning to slightly bluer tones at the outer edges, indicating ongoing, but reduced, star formation activity in the galaxy's outer regions. There is no apparent spiral arm structure or distinct dust lanes visible, implying that it is likely an early-type galaxy. The galaxy appears to be isolated with a fairly indistinct, smooth halo. There are no visible signs of active galactic nuclei activity or a recent major merger event, although there are some signs of minor irregularities and disturbances in the galaxy's outskirts.