This galaxy presents as a relatively smooth, lenticular or early-type spiral, likely at a considerable distance. The central bulge is quite prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The light is concentrated in the central region, and the object is elongated with a high degree of symmetry. The outer regions display a bluer tint, possibly indicating more recent or ongoing star formation, though this activity appears to be subdued. There are no obvious signs of strong tidal interactions or major disturbances affecting its overall structure, although subtle perturbations cannot be ruled out. The overall impression is of a well-established galaxy in a relatively quiescent state.
