The galaxy exhibits a smooth, centrally concentrated morphology, with a predominantly round shape. The core displays a bright, yellowish hue, indicative of an older stellar population. The outer regions of the galaxy appear more diffuse and exhibit a slightly bluer tint, suggesting the presence of some younger stars. There is a hint of a faint, extended disk or a more complex structure, which is consistent with it having a red shift of 0.148425. The system shows no obvious signs of major interaction or ongoing merger activity, though a possible minor disturbance can't be ruled out.
