The galaxy presents as a moderately luminous, elongated object with a smooth, diffuse appearance. The light distribution suggests a somewhat spheroidal morphology, transitioning towards a disk-like structure. There is a subtle color gradient; the central region exhibits a slightly yellower or orange hue, potentially indicating an older stellar population, while the outer regions appear somewhat bluer, possibly hinting at more recent star formation. The galaxy appears relatively undisturbed, without any obvious signs of ongoing major mergers or tidal interactions. The overall impression is of a galaxy in an intermediate stage of morphological evolution, possibly a lenticular or early-type spiral galaxy.
