The galaxy presents as a centrally concentrated, luminous object with a smooth, symmetrical morphology. Its form appears predominantly elliptical, exhibiting a high degree of sphericity, though precise shape determination is limited by the image resolution. There's no indication of spiral arms or a distinct disk structure. The galaxy core displays a bright, unresolved nucleus. The overall color profile suggests a population of older stars, with a yellow to reddish hue in the central region, becoming slightly bluer in the fainter outer regions. There's no visible evidence of tidal disturbances, major mergers, or active star-forming regions within the galaxy, suggesting it has undergone a period of relative quiescence. The galaxy is isolated, without apparent interactions with any neighboring galaxies.
