This galaxy presents as a moderately inclined spiral galaxy with a dominant central bulge. The bulge exhibits a yellow-orange hue, suggesting an older stellar population. The disk surrounding the bulge shows a bluer color, indicative of ongoing star formation and younger, hotter stars. The spiral arms are not well-defined, appearing somewhat flocculent and less tightly wound. The overall morphology suggests an intermediate spiral type. The galaxy appears relatively smooth, with only minor signs of disturbances or merging activity. There seems to be a low amount of star formation activity. The elliptical light distribution indicates it is significantly elongated.
