This galaxy exhibits a disk-like morphology, viewed at a moderate inclination. The central bulge appears prominent and exhibits a yellowish hue, likely indicative of an older stellar population. The disk shows hints of spiral structure, with bluer regions suggestive of ongoing star formation. A redder region is visible on the left side of the galaxy, perhaps a dust lane or HII region. The overall appearance suggests a galaxy undergoing moderate star formation with a substantial, evolved stellar population in its bulge. No obvious signs of major merging are present.
