The galaxy presents a primarily smooth morphology, with an apparent lack of distinct spiral arm structures or a prominent galactic bar. It exhibits a centralized concentration of light, indicative of a substantial bulge component or a possible active galactic nucleus. The overall shape approximates a slightly elongated spheroid, leaning towards round rather than cigar-shaped. There is a subtle color gradient, transitioning from a brighter, yellowish-white core to a slightly bluer halo surrounding it, suggestive of a moderate level of recent star formation in the outer regions, and a larger population of older stars toward the center. Indications of minor gravitational disturbances are potentially visible in the form of slight asymmetries in the outer halo, but no major merging events are immediately apparent. The galaxy's integrated light suggests it is a relatively massive system, though star formation is not particularly vigorous at this observed point in its evolution.
