The galaxy appears as a somewhat diffuse object, exhibiting an elliptical morphology. The light distribution suggests a relatively smooth profile, hinting at a lack of significant spiral arm structure or prominent dust lanes. There is a suggestion of a bulge, with a more intense and yellowish core, indicating a possible concentration of older stellar populations. There's a slight elongation, but the galaxy is generally moderately rounded. The outer regions appear fainter and bluer, potentially indicating ongoing, though low, levels of star formation at the outskirts. There is some suggestion of disturbance in the disk, which could be due to a minor gravitational interaction, although it appears primarily undisturbed. The overall color of the galaxy is moderately red-shifted, indicating that the galaxy is relatively distant.
