The galaxy appears to be a spiral galaxy with a prominent disk structure. There is evidence of well-defined spiral arms. The central bulge is moderately sized and has a yellowish hue. A significant portion of the galaxy appears to be undergoing star formation, as evidenced by its luminosity and the presence of spiral arms. There is no clear evidence of any major mergers or significant tidal disturbances. The galaxy exhibits a moderate inclination angle relative to our line of sight.
