The galaxy presents as a single, largely homogenous object. It exhibits a generally elliptical morphology, appearing mostly smooth in texture without prominent spiral arms or a central bar structure. There is some indication of slight asymmetry, with a subtle elongation along one axis.

The color profile suggests a population of older stars, with a concentration of light toward the redder end of the spectrum. There is faint evidence of bluer regions, implying some ongoing, but limited, star formation. No apparent dust lanes or significant gas obscuration are visible. The galaxy's luminosity suggests it is a massive system, yet the lack of significant structural features might indicate it is approaching a quiescent state in its evolution. There is also some distortion, hinting at minor interactions with other galaxies.
