The galaxy presents a generally smooth morphology, appearing as a lenticular system. It exhibits a concentrated, bright central bulge that is primarily yellow-orange in color, suggesting a population of older stars. The disk is relatively featureless, with a faint greenish hue, possibly indicating some ongoing, though weak, star formation. The galaxy is elliptical in shape, exhibiting a moderate degree of flattening and possibly some minor disturbance in its structure. There are no signs of prominent spiral arms or bars. The overall color profile suggests that the stellar population is dominated by older stars, but with some presence of younger stars. There is a possible merging event occurring.
