The galaxy presents as a relatively compact object with a dominant central bulge exhibiting a high degree of luminosity. There is a noticeable disk component surrounding the bulge, which appears somewhat irregular and potentially disturbed. The disk displays variations in color, suggesting differing stellar populations or dust distribution. The bluer hues in some regions of the disk may indicate ongoing star formation. There is an indication of minor distortions within the galactic structure, possibly resulting from interactions or mergers. The galaxy appears to be a relatively low-redshift object given its discernible features. Overall, the morphology suggests a galaxy undergoing some form of disturbance or interaction, impacting its structure and star formation activity.
