The galaxy presents as a relatively smooth, centrally concentrated object with an overall elliptical morphology. Its color suggests a population of older stars, with a notable absence of blue hues indicative of recent star formation. There is a very slight asymmetry in its shape, possibly suggesting a past or ongoing minor interaction or merger event. A faint halo or extended envelope is visible around the main body of the galaxy, suggesting a diffuse stellar population extending beyond the core. The galaxy appears to be relatively undisturbed, showing no strong tidal features or signs of active galactic nuclei activity based on its color. There are possible faint irregularities within the galaxy, suggestive of substructure or recent accretion.
