The galaxy presents an elongated, cigar-shaped morphology. A central, brighter region exhibits a yellowish-orange hue, potentially indicating an older stellar population or dust obscuration. Emanating from this core are fainter, reddish extensions or tails, possibly indicative of tidal features or ongoing star formation regions. There appears to be some blue-ish regions as well, these could also be a site of star formation. The overall light distribution suggests a relatively smooth structure, though some subtle irregularities are visible within the outer extensions. There is no clear evidence of a spiral arm structure.
