The galaxy presents as a moderately inclined spiral, exhibiting a prominent central bulge that graduates smoothly into a disk. The bulge appears yellowish-orange, suggestive of an older stellar population. The disk shows signs of spiral arms, though they are somewhat ill-defined and flocculent, with a bluer tint indicating the presence of younger, hotter stars in these regions. The overall color profile suggests a system with ongoing, but perhaps subdued, star formation. There appears to be some minor asymmetry or irregularity at the extreme ends of the galaxy, possibly indicative of past interactions. No bright, discrete star-forming regions or intense HII regions are clearly visible within the disk. The galaxy's smooth overall appearance suggests that it is relatively undisturbed and not currently undergoing a major merger event.
