The galaxy presents as a somewhat smooth, lenticular structure, exhibiting a subtle disk-like morphology. The light distribution indicates a centrally concentrated luminosity profile. The galaxy displays a color gradient, with a slightly bluer hue in the outer regions and a more pronounced red color towards the core, possibly indicating a difference in stellar populations. There is no obvious spiral structure present. The galaxy exhibits a minor disturbance that may be an indication of interaction with a smaller galaxy. The intermediate roundness suggests the disk is inclined relative to our line of sight.
