The galaxy appears to be a relatively smooth, elliptical system. Its overall form is elongated, with an axis ratio suggesting it is viewed at an intermediate inclination. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. There is little evidence of strong spiral arm structure or prominent dust lanes. A slight asymmetry is observed in the outer regions, potentially indicating a minor disturbance or interaction. The galaxy's color is largely uniform, with a slightly bluer hue in the central region suggesting the presence of younger stellar populations, although the overall color is consistent with an older stellar population. Some irregular light surrounding the galaxy may suggest there could be a recent or ongoing merger.
