The galaxy presents as a luminous, elliptical morphology. A bright, concentrated central bulge dominates the structure, indicating a high stellar density in this region. The galaxy exhibits a relatively smooth appearance, with little to no visible spiral arm structure or significant dust lanes. The color profile is generally consistent throughout, suggesting an older stellar population with minimal ongoing star formation. The galaxy's light is more concentrated in the redder wavelengths, indicative of a population of older, redder stars. A faint, extended halo surrounds the central region. The overall shape of the galaxy is not perfectly circular but is somewhat elongated. There are no obvious signs of major tidal disturbances or recent merger activity, however minor disturbances cannot be ruled out.
