The galaxy appears to be a spiral type, characterized by a prominent central bulge and a relatively well-defined disk. The spiral arms are tightly wound and quite prominent. Evidence suggests the presence of a bar structure spanning across the central region of the galaxy. The bulge appears moderate in size and shows a yellowish hue, potentially indicating a population of older stars. The disk exhibits a bluer color, suggesting ongoing star formation.  The galaxy has a slightly elongated appearance. There is no evidence of a major ongoing merger, though there is a slight asymmetry.
