The galaxy appears to be a relatively smooth, elliptical system. It is characterized by a centrally concentrated bulge that dominates the overall light distribution. The light tapers off gradually from the center, showing a fairly regular profile with no obvious spiral arm structures or a distinct disk component. There are no visible dust lanes. The galaxy appears to be slightly more elongated than perfectly spherical. The object exhibits colors indicating older stellar populations are prevalent. There is a hint of a slightly reddish hue in some regions of the galaxy suggesting the presence of evolved stars. No significant tidal features or signs of major recent merger events are immediately apparent in this image, although subtle disturbances cannot be ruled out.
