The galaxy presents as a relatively bright, well-defined elliptical or lenticular structure. It appears predominantly smooth in texture, with a high degree of central concentration. A subtle disc-like feature is oriented edge-on, bisecting the central bulge. This disc structure shows a slightly bluer hue relative to the central bulge, possibly indicating some ongoing, although modest, star formation within the disc. The galaxy has a generally rounded morphology, showing no obvious signs of major tidal disruption or ongoing merger activity, although it is possible there is minor disturbance. Its color indices suggests the presence of an older stellar population.
