The galaxy presents as a relatively compact, elliptical morphology with a smooth light distribution and minimal discernible features. The central region appears to exhibit a high concentration of light, suggestive of a prominent galactic nucleus. There is no evident spiral structure, bar, or dust lanes, and the overall color profile is consistent with an older stellar population. Faint, diffuse light extends outwards from the core, forming a roughly spherical halo. No signs of ongoing major mergers or significant tidal disturbances are visible. The galaxy appears to be relatively isolated within its field.
