The galaxy presents an overall smooth morphology, with a near-spherical appearance. The light profile appears centrally concentrated with a diffuse, extended halo. There is a slight elongation, but it is difficult to discern any clear spiral structure or distinct features. Color gradients are subtle, with the central region exhibiting a yellower hue compared to the outer regions which appear slightly bluer. This may suggest a population of older stars in the core and younger stars at the outskirts. There is no obvious evidence of a major ongoing merger, although the possibility of a minor interaction or past disturbance cannot be ruled out given the irregular features in the light distribution. Overall, this appears to be a relatively evolved galaxy undergoing some star formation.
