The galaxy appears to be a relatively compact object. Its overall color profile suggests a significant degree of star formation, indicated by the presence of bluer hues dominating the central region. A distinct, bright core is visible, suggesting a high concentration of stars or potentially an active galactic nucleus. While the main body of the galaxy seems to be fairly homogenous, there is a slight suggestion of a disturbance or possible merging event in the galaxy's profile. The galaxy lacks distinct spiral arms, instead appearing more amorphous, which coupled with the merging signatures, may indicate a system undergoing a significant morphological transformation or interaction.
