The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. It exhibits a slightly elongated, roughly elliptical shape. The central region displays a bright, yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the galaxy fades in intensity, with a subtle color shift towards a greenish-blue tinge in the outer regions. This may indicate the presence of younger, hotter stars in the galactic disk. There is little evidence of spiral arm structure or significant dust lanes. The overall appearance is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy with some ongoing, but relatively low, star formation in the outer regions. There do not appear to be any obvious signs of any major merger events or tidal disturbances.
