The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, exhibiting a slightly elongated, cigar-like shape. Its overall color suggests an older stellar population, with a dominant yellowish hue throughout the main body of the galaxy. There is little evidence of prominent spiral arm structure or significant dust lanes. The light is concentrated in the center, which indicates a centrally concentrated mass distribution. Minor disturbances could be present within the galaxy's morphology, but it does not appear to be undergoing a major merger or significant tidal interaction. 
