The galaxy presents a morphology that is somewhat smooth in appearance, though with subtle features that disrupt a purely elliptical or lenticular classification. The galaxy exhibits a moderate degree of internal structure, with hints of disk-like features or spiral arms, though these features are not clearly defined or prominent. There may be subtle signs of a past interaction or minor disturbance of the galaxy's structure. The overall light distribution appears relatively centrally concentrated, with a gradual falloff in surface brightness toward the outer regions. There is evidence of recent star formation in the galaxy, as traced by the galaxy's color and patchy regions of blue light. However, this star formation appears relatively limited in spatial extent. The galaxy's color suggests it is not particularly rich in dust.
