The galaxy presents as an elliptical or lenticular type, with a relatively smooth, featureless morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region residing in the core. The galaxy's overall shape appears somewhat elongated, tending toward a cigar shape. There is no obvious indication of spiral arm structure or a prominent disk. The color distribution suggests an older stellar population, with a yellowish-orange hue dominating the central bulge, while bluer regions are faintly visible towards the galaxy's periphery, which indicates recent star formation may be occurring, but at a low rate. There is no strong evidence of recent or ongoing merger activity, though some minor disturbance cannot be entirely ruled out. The overall appearance indicates a galaxy with a significant stellar mass.
