The galaxy presents as a somewhat smooth, centrally concentrated object, displaying characteristics intermediate between elliptical and lenticular morphologies. Its overall form is elliptical, but not perfectly spherical, tending towards a moderately flattened shape. A prominent bulge region dominates the galaxy's core, exhibiting a smooth, relatively high surface brightness. The outer regions of the galaxy gradually fade into the background sky, displaying a less structured halo. There is minimal evidence of well-defined spiral arms or distinct dust lanes. Color gradients are subtle, with the central bulge appearing slightly redder than the outer regions, suggesting an older stellar population in the core. No obvious signs of ongoing major mergers or tidal disturbances are apparent, although subtle asymmetries may indicate minor interactions or internal dynamical processes. The overall impression is of a relatively evolved galaxy with a modest rate of star formation.
