The galaxy appears as a moderately bright, extended object. Its morphology is somewhat disturbed, with no clear spiral arm structure discernible. The central region exhibits a concentrated yellowish hue, possibly indicative of an older stellar population or significant dust obscuration. The outer regions show a more diffuse and irregular shape, with hints of bluer light, potentially signaling ongoing star formation. There may be some tidal features or minor disturbances, suggesting a possible interaction or past merger event. The galaxy displays an overall asymmetrical structure.
