The galaxy presents a generally smooth morphology, with a centrally concentrated brightness profile. The core exhibits a yellowish-white hue, suggesting an older stellar population. There is a very slight elongation present, but it is overwhelmingly rounded in appearance. The outer regions of the galaxy appear redder, potentially indicating a difference in stellar population or dust content compared to the core. There's no strong evidence of spiral arms or prominent features. It appears largely undisturbed and shows no obvious signs of a recent major merger, although slight disturbances cannot be ruled out. Star formation appears to be quite low. Overall, this galaxy is consistent with a relatively massive elliptical galaxy.
