The galaxy presents as an elongated, lenticular or disk-shaped structure, oriented nearly edge-on relative to our line of sight. There is a prominent central bulge that appears relatively smooth and spheroidal, with a concentrated bright yellowish-white hue, suggesting an older stellar population.

Surrounding the bulge, the galactic disk is visible as a fainter, extended structure. The disk appears relatively thin and flat, with a slight gradient in color moving outward from the center. The extremities of the disk exhibit a somewhat diffuse edge, and a change from yellowish white to orange, which might signify increasing presence of older stars and/or dust. The image suggests a galaxy that is not currently undergoing significant star formation. The overall smooth appearance and lack of prominent spiral arms or distinct features suggest a relatively evolved system, potentially on the red sequence. There is no evidence of recent merging activity or significant tidal disturbances.
