The galaxy appears to be a relatively smooth, elongated structure. It exhibits a prominent central bulge that is more concentrated and displays a yellowish hue, indicative of an older stellar population. Surrounding the central bulge is a disk component, displaying a slightly bluer color, suggesting the presence of younger stars and ongoing star formation, albeit at a relatively low rate. The galaxy's overall shape leans towards being cigar-shaped, with a slight inclination relative to the line of sight. There is no evidence of significant ongoing merger activity or major disturbances to its structure.
