This galaxy appears to be a spiral galaxy, presenting a face-on orientation relative to our line of sight. It exhibits a diffuse, disk-like structure with a somewhat irregular morphology, showing evidence of potential interactions or disturbances. The galaxy's color profile suggests a mix of stellar populations, with the central regions displaying a more yellowish hue possibly indicating an older population, while the outer regions show a bluer tint, suggestive of more recent star formation activity. There is a suggestion of spiral arm structure, but its prominence is diminished, potentially due to the galaxy's distance or ongoing interactions. Faint, irregular extensions are observable, possibly tidal features resulting from gravitational interactions with a neighboring galaxy. Overall, the galaxy appears to be relatively small in size, with a moderate mass and a subdued rate of star formation.
