The galaxy presents a slightly inclined disk structure. A prominent central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. The disk component shows a bluer tint, indicative of younger stars and ongoing star formation. There are some indications of spiral arm structure, although the image resolution limits detailed tracing. The galaxy appears relatively undisturbed with no obvious major merger signatures, although minor disturbances cannot be ruled out based on this image alone. Overall, the galaxy presents characteristics consistent with an intermediate type spiral galaxy undergoing moderate star formation.
