The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus. Extending outwards from this central core, a fainter, more diffuse region is observed, potentially representing the galactic disk or bulge. There appears to be a smooth, relatively featureless morphology, with no clear spiral arm structures or prominent dust lanes visible in this image. A blueish hue permeates the outer regions, indicative of a population of younger, hotter stars. The overall morphology suggests this galaxy is likely an elliptical or lenticular type, viewed at a significant inclination. The apparent lack of significant disturbances hints at a relatively quiescent state, with no signs of recent major merger events.
