The galaxy presents as an elongated, somewhat cigar-shaped object. A smooth, centrally concentrated bulge dominates the morphology, exhibiting a yellowish-orange hue, suggesting an older stellar population. Fainter, diffuse extensions of bluish light emanate from either end of the central bulge. These extensions hint at the presence of younger stars. There is little evidence of defined spiral arms, dust lanes, or active star-forming regions within the main body of the galaxy. No signs of any major mergers or tidal disturbances are observed in this image. The overall appearance suggests a relatively evolved galaxy with a moderate stellar mass.
