The galaxy presents a complex morphology, suggestive of a possible interaction or merger event. The primary body of the galaxy appears somewhat elongated and diffuse. There is a bright central bulge which seems to be composed of older stars, indicated by its yellower hue. The galaxy exhibits faint spiral arm-like structures. There is also a hint of blue within these structures, indicative of ongoing star formation. The galaxy has a redshift of approximately 0.088, placing it at a considerable distance. There is a suggestion of disruption to the main galactic structure. Some areas have been interpreted as signs of minor disturbances, though a merger of components has also been suggested, with a significant amount of disk present. The estimated stellar mass of the galaxy is large, suggesting it is a mature system. Star formation rate is low to moderate, and the specific star formation rate is quite low. The galaxy displays notable luminosity in the g, r, and z bands, indicating a substantial stellar population.