The galaxy presents as a relatively bright, disk-shaped structure. The central bulge appears prominent and exhibits a yellowish-white color, suggesting a population of older stars. The surrounding disk is less defined and appears more diffuse, with a bluer tint on the periphery, hinting at the presence of younger, hotter stars and possibly ongoing star formation. The galaxy's overall form suggests a transition between a spiral and lenticular type, potentially with faint, tightly wound spiral arms that are not clearly resolved in the image. The galaxy's elongation indicates a non-spherical shape; it is more cigar-shaped than fully rounded. There are no obvious signs of recent major mergers or tidal disturbances. The galaxy shows a moderate amount of star formation activity.
