The galaxy appears to be a relatively smooth, elliptical or lenticular type. It is characterized by a central bright region indicative of a significant concentration of stars. The light profile suggests a primarily spheroidal shape, with little to no evidence of spiral arms or a prominent disk structure. The color gradients show a slightly bluer core, possibly due to a small amount of residual star formation in the nucleus, transitioning to redder colors in the outer regions, suggestive of an older stellar population. There is also a hint of tidal disturbance, possibly from a minor merger event in the past.
