The galaxy exhibits a generally smooth morphology, with a discernible elongated shape, appearing somewhat cigar-shaped. There's a suggestion of a slight tidal disturbance or possible minor interaction event. The color distribution indicates a central concentration of older stellar populations, exhibiting a yellowish hue, grading outwards into somewhat bluer regions, suggesting more recent, ongoing star formation. The galaxy is not perfectly symmetrical, with hints of asymmetry in its outer regions. Overall, the galaxy appears to be in a transitional phase, potentially between a disk-dominated and spheroid-dominated morphology, with indications of past or ongoing minor mergers affecting its structure and star formation history.
