The galaxy exhibits a predominantly smooth morphology, appearing as a diffuse, elongated structure. Its overall shape is somewhat cigar-like. The central region displays a yellowish hue, suggesting an older stellar population, while a redder region is observed on one side, potentially indicating ongoing star formation. There appears to be some minor distortion of the galaxy's shape, suggesting a possible interaction or minor disturbance. There is no clear evidence of a well-defined spiral structure or prominent dust lanes. The galaxy's light distribution is centrally concentrated, fading gradually towards the outer edges.
