The galaxy presents an overall smooth morphology, with a relatively concentrated central region. The shape appears to be in between round and elliptical. There is a suggestion of a slight disturbance or irregularity in the outer regions, possibly indicating a minor interaction or internal process. The color distribution shows a gradient, with the central region exhibiting a bluer hue, potentially indicative of younger stellar populations or ongoing star formation. The outer regions appear redder, suggesting older stellar populations. The galaxy does not exhibit a prominent disk structure.
