The galaxy presents as a prominent, disk-shaped structure. It appears to be oriented at a moderate inclination relative to our line of sight. The central bulge is clearly visible and exhibits a concentrated brightness, suggesting a high density of stars. The disk component shows evidence of spiral arm structures, though they are not sharply defined. The color distribution suggests older stellar populations are more prominent within the bulge, appearing yellow in contrast to the disk. The disk exhibits patches of bluer light, which are indicative of younger, hotter stars and regions of ongoing star formation. There appears to be some disturbance present which may indicate a minor merger event, and the lower area of the galaxy shows hints of diffuse, irregular structure, potentially resulting from tidal interactions. The overall structure suggests a galaxy undergoing some form of evolutionary process, whether through internal dynamics or external interactions.
