The galaxy presents as a relatively smooth, elongated object. Its morphology is more akin to an elliptical galaxy, although a subtle disk-like structure may be present. The central region displays a significantly higher surface brightness compared to the outer regions, suggesting a concentration of older stars or an active galactic nucleus. The overall color of the galaxy appears redder compared to galaxies exhibiting high rates of star formation, potentially indicative of an older stellar population. The galaxy does not exhibit prominent tidal features or evidence of a major ongoing merger. There appears to be an asymmetry in the halo of the galaxy, suggesting possible minor interaction. The rate of star formation appears low, but has a wide range of uncertainity.
