The galaxy presents as a moderately bright, relatively compact elliptical structure. Its overall form appears largely spheroidal, exhibiting a smooth, featureless morphology with no apparent spiral arms or bar. There is a slight elongation to the shape, though it is predominantly rounded. The core region displays a higher concentration of light, gradually fading towards the outer edges. Color gradients across the galaxy are subtle, with a reddish hue predominating, suggesting an older stellar population. There is no evidence of significant dust lanes or recent star formation activity. The overall impression is of a mature galaxy, possibly undergoing passive evolution. No signs of merging or tidal disturbances are apparent within the immediate vicinity.
