The galaxy presents as a somewhat rounded, centrally concentrated system. It appears relatively smooth in texture, with no obvious spiral arm structures or significant dust lanes visible at this resolution. A dominant central bulge exhibits a yellowish-orange hue, suggesting a population of older stars. The outer regions of the galaxy fade into a bluer color, perhaps indicating some ongoing, though potentially limited, star formation activity in the outskirts. Overall, the morphology appears largely undisturbed, without significant signs of recent mergers or tidal interactions. The color gradient suggests a decline in stellar age and potential star formation rate with increasing distance from the galactic center.
