The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution appears largely uniform, suggesting a dominant spheroidal component. There is a subtle color gradient observable, transitioning from slightly bluer hues in the faint outer regions to yellower and redder tones towards the core, hinting at potential variations in stellar populations or dust content. A very small amount of irregularity may be present, but there is no significant evidence of spiral arms or a distinct disk structure. Any ongoing star formation appears low. The overall structure suggests a relatively evolved system.
