The galaxy appears to be a relatively smooth, elliptical-like object, exhibiting a fairly concentrated light profile. There is no obvious indication of spiral arms or a distinct disk structure. The galaxy appears moderately luminous. The central region of the galaxy exhibits higher intensity light emission. There might be a very faint hint of minor tidal disturbances. The galaxy does not appear to be undergoing a major merger, displaying a single, coherent structure rather than multiple distinct components. The overall color of the galaxy suggests a population dominated by older stars.
