The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentration of light, appearing a yellowish-orange hue, suggesting an older stellar population. Moving outwards from the core, there is a gradual decrease in surface brightness. The outer regions display a bluer tint in contrast to the core, suggestive of a population of younger, hotter stars although they are not as prominent. The galaxy’s overall form appears somewhat elongated. There are no obvious signs of spiral arms or a distinct disk structure. No significant tidal disturbances or indications of a major merger event are observed. The outer edges do not exhibit any bright clumps of star formation regions. Overall, the galaxy has a well-defined, consolidated appearance.
