The galaxy presents as a moderately bright, elliptical structure. It exhibits a smooth, concentrated light profile with a higher intensity core region that gradually fades towards the outer edges. There's a subtle elongation, suggesting an oblate spheroidal shape rather than a perfectly spherical one. The galaxy's color appears relatively uniform across its body, with a slight tendency towards the redder end of the spectrum. This implies an older stellar population with limited ongoing star formation. There are no distinct spiral arms, dust lanes, or other features indicative of active disk structures. Overall, the morphology appears to be that of a relatively evolved and quiescent system.
