The galaxy presents as a fairly compact, unresolved object. Its morphology appears smooth and largely featureless at this resolution. The light distribution suggests a spheroidal shape, with a high degree of circular symmetry. There is a gradual decline in luminosity from the core outwards, lacking any distinct spiral arm structures or a prominent disk. The galaxy exhibits a color gradient, appearing bluer at the core and becoming redder towards the outer regions. There are no apparent signs of tidal tails or distortions indicative of recent major merger activity. Minute irregularities surrounding the main body possibly suggest minor disturbances. Overall, it seems to be a relaxed system, possibly an elliptical galaxy or a lenticular galaxy viewed face-on.
