The galaxy presents as a concentrated spheroid of light. Its core appears a bright, uniform yellow, indicative of an older stellar population. The overall form is largely smooth and elliptical, with a high degree of roundness. No spiral arms, bars, or significant dust lanes are visible. There are no signs of ongoing major merger activity or significant tidal disturbances. The galaxy's light profile suggests a single dominant component with no apparent secondary nucleus or disrupted structure. Faint wisps of light extend from the central region, potentially representing a very tenuous and diffuse halo. Its colour suggests a galaxy that is not very actively forming stars.
