The galaxy presents as a lenticular or possibly an edge-on spiral, appearing elongated in shape. There is a distinct central bulge region of brighter luminosity which fades into a more diffuse outer disk. Within this brighter region, I observe a smooth luminosity gradient, without any indication of spiral arm structure or dust lanes. The overall color appears to be relatively blue-white, suggesting a population of younger stars, especially in the area outside the central bulge. There are some indications of a possible disturbance to the morphology of the galaxy, with a faint extension visible on one side of the disk. Further investigation of this feature at different wavelengths would be beneficial to determine its true nature. The galaxy exhibits a medium redshift, indicating a considerable distance and substantial luminosity. Its mass is estimated to be high. The star formation rate is low, relative to its mass.
