This galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with an approximate effective radius of 4.5 kpc. The galaxy's core is bright and yellowish, potentially indicating a population of older stars. Moving outward from the core, the color becomes slightly bluer and fainter. There may be some disk-like features embedded within the structure. I do not observe any obvious signs of ongoing major mergers. Minor asymmetries exist in its outskirts, suggestive of possible minor interactions or internal dynamics causing slight disturbances. The integrated light suggests a galaxy of considerable luminosity, given its inferred distance. Star formation is ongoing, but at a low rate. I estimate the galaxy to contain a substantial amount of stellar mass.