The galaxy presents as a relatively compact object with a bright, concentrated central region. The morphology appears largely spheroidal, exhibiting a smooth light distribution in the inner regions. Fainter, more diffuse light extends outwards from this central concentration, forming a faint halo. The dominant color is bluish-white, suggesting a population of younger, hotter stars, though the presence of redder hues in the outer regions indicates the presence of an older stellar population as well. There appears to be a slight asymmetry in the outer regions, possibly indicating a minor gravitational interaction or disturbance. There is no indication of prominent spiral arms or a strong bar structure. Overall, the galaxy gives the impression of being a fairly massive, evolved system with ongoing, albeit potentially low-level, star formation.
