The galaxy appears to be a spiral galaxy viewed at a significant angle relative to its disc, giving it an elongated or cigar shape. A prominent central bulge is observed with a yellowish color, possibly indicating an older stellar population within. The galaxy exhibits a faint disk structure with what may be some spiral arm features. The galaxy exhibits an overall smooth appearance. There is no sign of recent major merger activity. The color gradient from the center outwards suggests some active star formation is occurring, albeit at a low rate.
