The galaxy presents as a single, largely homogenous structure. The light profile appears centrally concentrated, with a smooth, gradual decline in surface brightness away from the core. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars, with potentially ongoing, but relatively low-level star formation.

The overall shape is nearly circular with a slight elongation. No distinct spiral arm structures or prominent dust lanes are visible. The outer regions display a bluer color, indicative of younger stellar populations within these areas. There is no evidence of any major ongoing mergers or tidal disturbances affecting the galaxy’s overall morphology, only slight disturbances.
