The galaxy presents as an elongated, cigar-shaped structure with a noticeable bulge. The central region displays a yellowish hue, possibly indicating an older stellar population and lower star formation rate. Extending outward from the center, faint bluish regions are visible, particularly at the extreme ends of the galaxy, which could indicate regions of more active star formation. There is some indication of minor disturbances in the surrounding stellar distribution. There appears to be little or no visible spiral structure or well-defined disk.
