The galaxy exhibits an elongated, cigar-like morphology. It appears to be a relatively smooth object, with subtle features. There are two main distinct regions, a more yellowish and brighter section on the left, and a fainter, slightly bluer region on the right. The left section may be the bulge. The overall structure suggests a galaxy undergoing a possible disturbance or interaction, though no major merger events are immediately apparent from the image. The galaxy has a notable size, implying a substantial stellar mass. Given its color profile, this galaxy is likely composed of older stellar populations and exhibits a low rate of star formation.
