The galaxy appears as a moderately luminous, flattened elliptical or lenticular system with a smooth, concentrated central bulge. There is a faint, diffuse disk component that is elongated, suggesting an edge-on or nearly edge-on orientation relative to our line of sight. The color gradient indicates an older stellar population. The galaxy shows no distinct spiral arm structure. The central bulge appears brighter and more yellowish, with a slight color gradient toward a redder hue in the outer regions of the disk, characteristic of a quiescent system with minimal recent star formation. There is no clear evidence of significant ongoing mergers or tidal disturbances. The overall structure appears relatively undisturbed and smoothly symmetric, consistent with a mature galaxy.
