This galaxy exhibits a predominantly smooth morphology, with a suggestion of some extended structure. The galaxy's core is characterized by a distinct reddish hue, indicative of an older stellar population, and potential dust obscuration. The outer regions show a transition to bluer colors, implying the presence of younger stars and ongoing star formation, though at a seemingly modest rate. There is a slight asymmetry, with indications of a possible minor disturbance in the gravitational structure, but generally the object appears to be relatively relaxed. It's a well-formed and cohesive object.
