The galaxy presents as a fairly smooth, elliptical object. Its core is characterized by a concentrated, bright yellowish-white luminosity, suggestive of an older stellar population. This central region fades gradually into a less concentrated, outer halo.

There's a slight elongation to the galaxy’s overall shape, but it remains generally round. No distinct spiral arms or prominent dust lanes are visible; instead, the overall structure appears relatively homogenous.

The galaxy displays a color gradient, with the core appearing more yellow-orange and the outer regions subtly trending towards redder hues. This is consistent with a stellar population gradient, where older, redder stars are more prevalent in the outskirts. The galaxy's overall appearance does not show any major disturbances from mergers. However, there is a subtle irregularity on the galaxy's periphery, potentially indicating past interaction with smaller galaxies or minor internal dynamics.
