The galaxy presents as a somewhat elongated structure, appearing cigar-shaped with an apparent major axis exceeding its minor axis. The central region exhibits a concentrated luminosity with a yellow hue, indicative of a population of older stars. Surrounding the core is a more diffuse region displaying a bluer color. This suggests the presence of younger stars or ongoing star formation within the outer disk, though at a low rate. There's a slight asymmetry evident in the outer regions, but no significant signs of tidal tails or significant morphological disturbance are visible, suggesting no major mergers. The overall morphology appears to be of a fairly regular and established galaxy. The distribution of light suggests a generally smooth profile, though the disk feature is seen. 
