The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and diffuse morphology. There is a concentration of light towards the center, suggesting a prominent bulge. The overall shape appears slightly elongated, with a ratio of major to minor axis modestly deviating from unity. No distinct spiral arms or prominent dust lanes are apparent. The galaxy possesses a moderate redshift, indicating a substantial distance. The color gradient suggests an older stellar population, particularly within the bulge, but the outer regions show evidence of recent star formation. There may be some minor asymmetry or disturbances in the outer regions, but these are not pronounced enough to suggest a major ongoing merger event. The galaxy's effective radius is approximately 4 kpc.
