The galaxy appears as a moderately bright object, exhibiting a generally smooth morphology. The central region presents a somewhat rounded shape. The overall color profile suggests a population of both young and old stars. There is a suggestion of slight asymmetry or minor disturbances in the galaxy's structure, hinting at possible past interactions or internal dynamics. The light profile appears relatively concentrated, with a gradual falloff from the core. There is some evidence of ongoing star formation. There may be a small merger happening, though if there is, it is minor.
