The galaxy exhibits an elongated morphology with a relatively smooth appearance overall. There appears to be evidence of a possible minor or major merger event based on visual disturbances or tidal features that may extend from the primary galactic body. The object is generally redder in appearance, possibly indicating an older stellar population or dust obscuration. There may be areas with bluer light, indicative of younger, hotter stars and possible star formation activity. The galaxy shape is between round and cigar shaped.
