The galaxy presents as a slightly disturbed disk galaxy, exhibiting a moderate degree of internal structure. Its overall morphology suggests a transition stage between a relatively smooth elliptical galaxy and a more defined spiral. The central bulge is prominent and appears relatively bright and concentrated. Surrounding the bulge is a fainter, bluer disk component with indications of loosely defined spiral arms or flocculent structures. There is evidence of some tidal features or minor disturbances, indicating possible interactions with a smaller companion galaxy or recent merger event. The galaxy exhibits a bluish hue, particularly in the disk region, suggesting ongoing star formation activity. Overall, the galaxy appears to be relatively low in mass, with a moderate star formation rate.
