This galaxy appears as a relatively compact object with a smooth morphology, and the light is dominated by warmer colors. It is approximately circular in shape and exhibits a radial concentration of light. The core region shows a prominent, concentrated luminosity with an orange hue, which is indicative of an older stellar population. There is a subtle gradient of decreasing intensity outward from the central bulge. There is no observable spiral arm structure or prominent dust lanes. The galaxy appears to be at a relatively high redshift, which suggests it is significantly distant and therefore, likely observed in an earlier stage of its evolution.
