The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a generally smooth morphology, with little evidence of distinct spiral arms or prominent dust lanes. The color profile suggests a dominant population of older stars, evidenced by the yellow-orange hue concentrated towards the central bulge. A subtle greenish tinge is observed in the outer regions, possibly indicating the presence of younger stars or ionized gas, though this is not definitively discernible. The isophotes are generally regular and concentric, lending to the impression of a well-relaxed system. There is no clear indication of recent major mergers or tidal disturbances within the immediate vicinity of the galaxy's main body. The overall impression is that of a relatively evolved galaxy, possibly with a low ongoing star formation rate.
