The galaxy presents a generally smooth morphology, appearing largely featureless in the available imagery. It exhibits a concentrated central region, with a gradual decrease in luminosity outwards. The object is nearly circular in appearance, showing minimal elongation. There is a slight color gradient, transitioning from a more yellowish hue at the core to a slightly redder color in the outer regions. Evidence of spiral arms or prominent dust lanes is absent, suggesting that the galaxy is likely elliptical or lenticular. No indications of major ongoing mergers or significant tidal disturbances are apparent. The object's overall characteristics suggest it is likely a massive galaxy with a moderate star formation rate.
