The galaxy presents a largely smooth and elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes within this particular image. The light distribution is concentrated towards the center, showing a bright, unresolved core. The galaxy displays a yellow-orange hue, suggesting an older stellar population, with redder stars dominating the light output. The galaxy appears to be relatively isolated, with no clear signs of major tidal disturbances or ongoing mergers. The shape appears generally round, with only a slight deviation towards a more elongated form. There is a hint of minor asymmetry in the outer regions, but it is not particularly pronounced.
