This galaxy exhibits a slightly elliptical morphology. The central region appears as a bright, concentrated bulge, emitting a yellowish light, suggestive of an older stellar population. Surrounding the bulge is a fainter, bluer disk component. The disk is not well-defined, lacking prominent spiral arm structures. There seems to be a relatively smooth transition from the central bulge to the outer disk regions. The overall color gradient suggests a mixture of stellar populations, with older stars dominating the central bulge and younger, bluer stars distributed throughout the disk. There may be some dust obscuration contributing to the patchy appearance of the disk. The galaxy does not show obvious signs of recent major merger activity, appearing relatively undisturbed.
