The galaxy appears as a somewhat elliptical, diffuse structure, possibly a disk galaxy viewed at an oblique angle. Its color suggests a mix of stellar populations, with a dominant yellowish-white hue indicating a significant population of older stars. There appears to be a bright central bulge that is more luminous compared to the outer regions. The outer regions fade gradually, indicating a relatively smooth density gradient. There are hints of subtle spiral arm structure. The galaxy shows hints of disturbances, possibly tidal features or minor mergers. Overall, the galaxy presents a relatively ordered structure with possible minor interactions, exhibiting moderate star formation.
