The galaxy appears as an elongated, lenticular structure. The central bulge exhibits a bright, concentrated glow with a slightly bluish tinge, which may indicate the presence of a population of younger, hotter stars. The outer regions display a smoother, more diffuse profile. This smoother profile with a lack of distinct spiral arms is also consistent with an elliptical or lenticular galaxy type. There is some minor evidence of possible faint and diffuse outer structures in the form of asymmetry, however overall the object appears relatively undisturbed. The galaxy appears relatively compact, with an estimated size of a few kiloparsecs. Overall, the galaxy displays a modest level of star formation activity, as is apparent by the light detected and central blue tinge. The object’s color indices suggest an intermediate redshift.
