The galaxy appears as a relatively smooth, elliptical-like structure. Its overall shape is quite rounded, with a slight deviation from perfect circularity. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer edges, suggesting a lack of distinct spiral arms or other prominent features. The color gradient across the galaxy shows a central yellowish hue transitioning to a slightly redder tinge in the outer regions. This color distribution may be indicative of an older stellar population dominating the core, with a potential presence of dust obscuration or a population of younger, bluer stars in the outskirts, albeit subdued. No signs of ongoing major mergers or significant tidal disturbances are readily apparent, but a minor irregularity or subtle asymmetry cannot be ruled out at this resolution. The morphology suggests a galaxy that has largely completed its major assembly phase.
