The galaxy presents as a diffuse, extended object with a slightly irregular morphology. A central, bright region dominates the light profile, exhibiting a yellowish-orange hue that suggests an older stellar population. Fainter, bluer extensions are visible extending in one direction suggesting a tidal feature possibly caused by a galaxy interaction. The galaxy appears relatively smooth in overall structure, with no distinct spiral arms or bar visible in the optical bands, indicative of an elliptical or lenticular morphology. There are two distinct regions with a strong color gradient, and the color gradient from the center to the edges of the object suggests a decrease in stellar age. The overall impression is that of a galaxy experiencing, or having recently experienced, some form of disturbance, whether it be a minor merger or some other form of gravitational interaction.
