The galaxy presents as a roughly elliptical structure with a prominent central bulge. The bulge appears yellowish-orange in color, suggesting a population of older stars. Surrounding the bulge is a fainter, bluer disk component. The disk is not particularly well-defined, and the galaxy lacks strong spiral arm structure. The overall color profile indicates that the galaxy is more evolved, with a lower rate of star formation. There is slight evidence of morphological disturbance, but the object does not exhibit signs of a major merger event. The shape appears somewhat elongated.
