The galaxy presents as a roughly elliptical, lenticular structure, appearing largely featureless across its visible extent. The light profile is generally smooth, lacking any distinct spiral arms or prominent dust lanes. There is a slight colour gradient visible, shifting from a warmer yellowish hue at the core to a cooler, bluer tinge in the outer regions. The galaxy appears relatively isolated, without clear signs of recent or ongoing mergers or tidal interactions with neighboring galaxies. There appears to be a slight disturbance in the light profile, as if there is some kind of minor event occuring nearby. The morphology suggests a relatively mature stellar population, consistent with a galaxy that has largely completed its major star formation phase.
