The galaxy presents a defined spiral structure. Two dominant spiral arms are visible, emanating from a bright, moderately sized central bulge. The arms exhibit a medium winding, extending outwards in a relatively open configuration.  The color suggests the presence of both older stellar populations in the bulge, as well as younger, bluer stars within the spiral arms. The galaxy's overall shape appears somewhat elliptical. There is no obvious evidence of any major mergers or significant tidal disturbances. The structure of the galaxy is overall fairly regular, suggesting it is not undergoing significant disruptive processes. There is a hint of a bar-like feature.