The galaxy presents a centrally concentrated, largely featureless appearance, with a dominant, smooth bulge component. Its shape is generally elliptical, tending toward a somewhat rounded morphology rather than a highly elongated, cigar-shaped one. There is no clear evidence of spiral arm structures or a well-defined disk. The galaxy exhibits a central region of enhanced luminosity, indicative of a higher concentration of stellar populations or potentially an active galactic nucleus. A subtle color gradient is observed, trending from a more yellowish-white core to a slightly bluer outer halo, which may indicate younger stellar populations present in the outer regions. No strong signs of major mergers or significant tidal disturbances are readily apparent, although the possibility of minor interactions cannot be entirely ruled out.
