The galaxy presents as an elliptical morphology, largely smooth in appearance with a high degree of central concentration. Its overall color is indicative of an older stellar population, leaning towards the redder end of the spectrum. The light is diffuse and lacks any apparent spiral arm structures or prominent dust lanes. There is no evidence of active star formation regions within the galaxy based on visual inspection. The galaxy appears isolated, showing no immediate signs of tidal interactions or major disturbances from other galactic bodies. A slight ellipticity is noticeable, though the structure leans toward a circular form. 
