The galaxy appears to be a relatively smooth, elongated object. Its central region exhibits a bright, concentrated luminosity, possibly indicating the presence of a substantial stellar population or an active galactic nucleus. The color profile suggests a redder hue overall, which could indicate an older stellar population or significant dust obscuration. There may be indications of a disk-like structure seen edge-on. No major disturbances are visible, suggesting the absence of recent major merger events. There is very little apparent structure or distinct features, supporting the classification as relatively smooth.
