The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears fairly uniform, lacking distinct spiral arms or prominent features. The color profile indicates an older stellar population, with a yellowish-orange hue dominating the galaxy's core, gradually fading towards the outer regions. There is no apparent active galactic nucleus or significant dust lane obscuration visible in this image. The overall morphology suggests a relatively quiescent galaxy, possibly an early-type system with minimal ongoing star formation. There is no indication of any merger event or tidal distortions. The galaxy is relatively isolated.
