The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a high degree of roundness and minimal evidence of a disk structure or spiral arms. The central region exhibits a bright, concentrated luminosity.

There is a subtle color gradient; the core appears more yellow-red, potentially indicative of an older stellar population. The outer regions show a slight blue tinge, hinting at the presence of younger stars, though at a very low rate. There is no indication of major disturbances.

The object displays minimal signs of tidal interactions or ongoing mergers. The galaxy appears relatively isolated and undisturbed.
