The galaxy presents as an elongated, cigar-shaped structure. Its overall morphology is largely smooth, exhibiting a central bulge and a faint, diffuse disk. Color gradients indicate a bluer hue towards the outer regions of the disk and a slightly redder core. There are some minor disturbances, possibly indicating past or ongoing interactions with another galaxy. Some degree of ongoing star formation is apparent, but the specific star formation rate is likely low and the overall structure suggests a system dominated by older stellar populations.
