The galaxy presents as a generally smooth, elliptical structure. There is a noticeable concentration of light towards the center, suggesting a prominent galactic nucleus. The galaxy appears to be an elongated spheroid, presenting a moderate ellipticity. The color profile appears largely uniform, with hints of redder hues in the central regions, which may indicate an older stellar population. There is no obvious indication of strong spiral arm structures or significant dust lanes. There are no strong indications of major mergers or tidal disturbances.