The galaxy presents as an elliptical structure, exhibiting a smooth light distribution with no apparent spiral arms or defined dust lanes. The core appears intensely luminous, gradually fading towards the outer edges, giving it a somewhat diffuse appearance. It appears mostly spheroidal, with a slight deviation from perfect circularity. The galaxy's color profile indicates an older stellar population, leaning towards redder hues with hints of yellow. There is no obvious indication of active star formation from the image, which is in line with the visual red color. There might be a very slight interaction, indicating that the galaxy could be involved in a potential minor merging event with a nearby object, based on the visual asymmetry of the galaxy's halo.
