The galaxy presents as a somewhat smooth, centrally concentrated object with an elliptical morphology. There is an apparent lack of prominent spiral arm structures or significant dust lanes within the visible spectrum. The central bulge appears brighter and slightly redder in color compared to the outer regions of the galaxy. A faint, diffuse halo extends outwards, suggesting a gradual decrease in stellar density with increasing distance from the galactic center. The galaxy's shape is more in-between round and cigar-shaped, leaning towards the rounder side. Overall, the galaxy's structure suggests it may be a relatively evolved system, potentially an elliptical or lenticular galaxy, exhibiting characteristics of a higher mass and relatively low ongoing star formation. There might be some minor disturbances, but the object does not appear to be undergoing a major merging event.
