This galaxy exhibits a predominantly smooth morphology, characterized by a centrally concentrated luminosity profile. The shape appears largely spheroidal, with a slight deviation towards ellipticity. There is no clear evidence of spiral arms or a prominent disk structure. The color gradient suggests a moderate population of older stars, with the central region potentially hosting a higher concentration of evolved stellar populations. Faint indications of minor disturbances can be seen at the very edges of the galaxy, suggesting a possible past interaction.
