The observed galaxy appears to be a relatively compact object with a centrally concentrated light distribution. The core region exhibits a bright, possibly unresolved source. Surrounding this is a more diffuse halo of light. The isophotes suggest a flattened, somewhat irregular morphology, possibly indicative of a disturbed system. There is no clear evidence of spiral arm structure or a well-defined disk. The outer regions of the galaxy show color variations, with hints of bluer regions and redder extensions, suggesting a mix of stellar populations and perhaps some ongoing star formation. There might be evidence of a minor tidal disturbance visible on either side of the main body of the galaxy. Overall, the system appears to be possibly an elliptical, with some ongoing mergers.
