The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. A distinct nucleus is apparent, exhibiting a bright, yellowish hue, indicative of a population of older stars. The surrounding halo appears more diffuse, with a bluer tint in its outer regions, suggesting the presence of some younger stars or ongoing star formation, albeit at a low rate. The overall structure lacks any pronounced spiral arms or bar features. The galaxy shows no signs of major interaction or disruption.
