The galaxy presents as a slightly elongated, lenticular or early-type spiral structure. It appears largely smooth in texture, with a dominant central bulge and a faint, diffuse disk component. There is no obvious spiral arm structure or prominent dust lanes visible. Color gradients suggest a redder, older stellar population dominating, particularly in the central regions. The overall luminosity indicates a relatively massive galaxy. There is potential, based on subtle distortions, that the galaxy is interacting or has interacted with another galaxy, but no merging or tidal features are clearly visible. The overall morphology suggests an older system with relatively low star formation activity, as evidenced by its redder color and lack of blue, star-forming regions.
