The galaxy presents as an elliptical or lenticular-like system, exhibiting a largely featureless and smooth morphology. It appears moderately concentrated, with no obvious spiral arm structures or a well-defined disk. The light distribution seems relatively uniform, with the central region displaying a somewhat brighter luminosity, fading gradually towards the outer edges. There is some evidence of disturbance in the system. The galaxy presents itself as a generally rounded object. The galaxy appears to be of average size, and is likely of significant mass. The light appears to be shifted towards the redder part of the spectrum, indicating a degree of redshift and suggesting considerable distance. The blue light indicates ongoing star formation within the system.
