The galaxy presents a somewhat amorphous structure, appearing neither purely elliptical nor distinctly spiral. A central bulge exhibits a concentrated luminosity, suggesting a significant population of older stars. The overall color profile indicates a leaning towards redder wavelengths, implying moderate star formation activity and a mature stellar population. There is a suggestion of a disk component with faint spiral arms, though these features are not sharply defined. The galaxy does not appear entirely undisturbed; the shape of the disk and arms appears slightly warped. There is no visible active galactic nucleus, or clear sign of being lensed.
