The galaxy presents as a flattened elliptical or lenticular structure, exhibiting a smooth, concentrated central bulge. The luminosity increases towards the core, suggesting a higher density of stars concentrated in that region. Fainter and more diffuse, extended disk-like structures are visible as very slight extensions along the major axis on either side of the center. These extensions are slightly bluer in color, suggestive of more recent star formation. No prominent spiral arms are discernible. The galaxy's overall color is yellowish-white to slightly bluish, transitioning to a more bluish hue toward the edges. There's a hint of possible minor tidal interaction or disturbance in the form of a slight irregularity in the outer envelope, suggesting the possibility of a previous interaction.
