The galaxy presents an elongated, somewhat disturbed morphology. A luminous central bulge dominates the galaxy's core, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Emanating from this central region are faint, diffuse arms or tidal features, visible as bluish and reddish extensions. The asymmetrical nature of these features hints at possible gravitational interactions, potentially a minor merger or tidal disruption event. There is a small region of blue nebulosity to the lower left which could be indicative of new star formation in this area. While a discernable disk structure is not immediately apparent, the overall morphology suggests a transitionary form, neither purely elliptical nor a well-defined spiral. This galaxy displays characteristics that imply a complex evolutionary history, possibly involving past interactions or mergers with smaller galactic systems.
