The galaxy presents as a moderately bright, lenticular or possibly early-type spiral system, viewed at a slight angle from face-on, such that the central bulge is visible. The central bulge is luminous and appears smooth, with a relatively high degree of roundness. It exhibits a blue hue, indicating the presence of some younger stellar populations, though the overall light profile suggests a system dominated by older stars. The outer regions display a fainter, disk-like structure that surrounds the central bulge. There is a subtle indication of minor disturbance or irregularity in the disk structure, and no obvious spiral arm structure is discernible, possibly due to the viewing angle or the galaxy's morphological type. Overall, the galaxy appears to be a relatively quiescent system, with a low star formation rate.
