The galaxy presents as a flattened elliptical morphology, appearing as a soft, diffuse glow with a relatively smooth light distribution. The central region exhibits a higher surface brightness, suggesting a concentration of older stellar populations. The galaxy displays an overall yellow-orange color, with some hints of bluer regions, implying a mix of stellar ages and potentially a low level of on-going star formation. The disk is not well defined, indicating an older galaxy with a smaller component of blue stars. The axial ratio suggests a significant flattening. No strong tidal features or signs of recent major mergers are readily apparent, although there appears to be a slight asymmetry in the outer regions, which could indicate minor interactions or disturbances. Overall, the galaxy appears to be relatively undisturbed and in a late stage of evolution.
