The galaxy exhibits a roughly elliptical morphology when viewed from our perspective. A bright central bulge is observed, suggesting a significant concentration of stars in the galactic nucleus. Surrounding this bulge, a fainter, more diffuse disk-like structure is visible. The galaxy displays a predominantly blue hue, particularly in the outer regions, which indicates the presence of younger, hotter stars and ongoing star formation activity. There appears to be some mild disturbance in the structure, but the overall shape suggests a relatively settled galaxy, though a minor interaction may be occurring.
