The galaxy presents as an elongated, disk-like structure, observed nearly edge-on from our vantage point. A prominent central bulge is evident, exhibiting a bright, yellowish hue. The disk itself appears relatively smooth, lacking distinct spiral arm features and a dusty appearance. The color gradient suggests a relatively older stellar population, primarily in the redder wavelengths, especially within the bulge. A slight asymmetry is observed within the disk, with what may be a slight warp or a potential tidal disturbance from a minor interaction. There is a hint of blue in the outermost regions of the disk, potentially indicating the presence of some younger stars. The galaxy appears to be in a relatively undisturbed state.
