The galaxy appears as a relatively compact object, approximately circular in projection on the sky. A bright, centrally concentrated region dominates the galaxy's light profile. Surrounding this core is a fainter, more diffuse halo or disk. There are indications of minor irregularities within the disk structure, perhaps suggesting tidal disturbances. These irregularities are subtle, not exhibiting the classic morphology of a major merger, but rather a slight distortion. Color gradients are present, with the central region appearing bluer than the outer regions, which have a noticeably redder color, possibly indicating an older stellar population in the outskirts. The overall appearance leans toward being relatively smooth, but with features that suggest interaction.
