The galaxy presents as a roughly elliptical structure, exhibiting a concentrated central bulge that appears yellow-orange in color. Moving outward from the core, the light profile diffuses gradually, transitioning into a more indistinct halo with a faint greenish-blue tinge. There is a subtle asymmetry in the distribution of light, suggesting a slight deviation from a perfectly smooth ellipsoid. No clear spiral arm structure or dust lanes are discernible in the image. The galaxy appears relatively isolated, lacking strong visual evidence of major ongoing mergers or tidal interactions with other nearby galaxies, though there are faint hints of disturbance in the outer regions. Overall, the galaxy appears to be an evolved system dominated by older stellar populations.
