The galaxy presents as a somewhat spheroidal structure with a smooth, diffuse light distribution. The core region exhibits a concentrated yellowish hue, indicative of an older stellar population. A subtle extension of bluer light emerges from the primary body, potentially signifying regions of more recent star formation within a disk-like component or a minor disturbance event. Overall the galaxy appears relatively isolated with no clear signs of a major ongoing merger event. However, there is evidence of some disturbance in the blue stellar structure.
