The galaxy presents as a yellowish-white elliptical system, exhibiting a largely smooth and featureless morphology. It appears relatively round, with a slight elongation, but no clear spiral arm structures are discernible. The central bulge is prominent, gradually fading into a less concentrated halo. There are hints of a possible merger event, with some irregularities in the outer regions of the galaxy, perhaps a tidal tail. Overall, the galaxy appears to be relatively evolved, consistent with a population of older stars.
