The galaxy appears to be a spiral galaxy viewed at a slight angle, not quite face-on. Distinct spiral arms emanate from a central bulge. The arms exhibit a clumpy structure, potentially indicative of ongoing star formation. The central bulge has a yellowish hue, suggesting a population of older stars, while the spiral arms show a bluer color, implying the presence of younger, hotter stars. The disk appears relatively thin. There is no clear evidence of a strong bar structure. Based on the slight asymmetries, there may be some minor gravitational interaction occurring with another galaxy, though no distinct companion is immediately visible. There does not appear to be any major ongoing merger event.
