The galaxy presents as a roughly elliptical object with a strong central concentration of light. A defined, though subtle, disk-like structure is present. The color distribution shows a shift towards redder hues in the core, transitioning to bluer colors in the outer regions of the disk. Indications of a possible tidal disturbance are present, potentially indicating past or ongoing interaction with another galaxy. The overall morphology suggests a possible intermediate type between an elliptical and a spiral galaxy with evidence of ongoing activity.
