The galaxy presents as a relatively smooth object, with a central, concentrated bulge that appears roughly spherical. The galaxy appears to be moderately luminous with a radial gradient extending from the core. Faint arms or extended features are not immediately apparent, nor is there evidence of a distinct disk structure. The color profile seems to indicate a more evolved stellar population, with hints of blue near the core. There may be ongoing star formation but the rate is moderate. There does not appear to be any significant sign of recent tidal interactions or mergers, although faint distortions are potentially present in the surrounding halo. The overall morphology seems to suggest an early-type spiral galaxy or a lenticular galaxy, but more detailed spectral analysis is needed to determine exact type and properties.
