The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular classification. The light distribution is concentrated towards the center, exhibiting a high degree of central symmetry. The primary body of the galaxy appears near circular. There is a slight asymmetry in the light distribution, perhaps indicating minor tidal disturbance or interaction, or internal dust lanes. The galaxy exhibits a color gradient, with a slightly bluer hue towards the outer regions. Overall, the galaxy appears relatively evolved with minimal signs of ongoing intense star formation.
