The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated, brighter luminosity with an orange-yellow hue, possibly indicating an older stellar population or significant dust content. Moving outward from the center, the luminosity decreases gradually. There is little evidence of distinct spiral arms or a well-defined disk. The galaxy exhibits an elliptical, somewhat irregular shape, possibly suggesting it may have undergone minor disturbances or interactions. The galaxy appears relatively isolated with no nearby companions visible within the immediate field, reducing the likelihood of major tidal interactions. The overall color gradient suggests a mature system with moderate star formation.
