The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a nearly circular profile. There is a subtle colour gradient noticeable, with a slightly bluer hue around the core, transitioning to redder tones toward the outer regions. This may indicate differing stellar populations, with younger stars being more prominent in the central region. There appears to be little or no discernible disk structure, and no prominent signs of spiral arms. There is no substantial evidence of recent or ongoing major mergers or tidal disturbances. Faint irregular light could be indicative of minor disturbances.
