The galaxy presents as a diffuse, elliptical object. Its core exhibits a bright, concentrated luminosity. The overall color is a muted yellowish-white, suggesting an older stellar population, though a faint bluer hue is detected towards the outer edges, suggesting the presence of some younger stars. The galaxy does not show any obvious spiral arm structures or a distinct disk. There are no clear indications of a major ongoing merger. A slight asymmetry or elongation is noted; This could indicate the presence of minor tidal disturbances or past interactions.
