The galaxy exhibits a disturbed morphology, suggesting a possible ongoing or recent interaction. The primary structure appears diffuse and somewhat irregular, with a smooth overall appearance but also some indications of disruption. Two bright central condensations are observed, which could be galactic nuclei in the process of merging, or regions of intense star formation triggered by the gravitational interaction. There are no well-defined spiral arms or a prominent disk structure that can be identified. The color is generally yellowish-orange. There appears to be limited evidence of active star formation within the galaxy, suggesting a relatively low star formation rate. The overall shape of the galaxy appears to be in between round and cigar shaped. Based on visual analysis, it is possible that a significant portion of the galaxy's mass is located within the two central bright regions.
