The galaxy presents as a roughly elliptical, though not perfectly spherical, form. A concentrated central bulge exhibits a strong yellowish-orange hue, indicative of an older stellar population. Moving outwards from the core, the light transitions into a dimmer, greenish glow, suggesting the presence of some younger stars, though overall star formation appears subdued. The outer regions display a faint, diffuse light that gradually fades into the background. There is no strong evidence of spiral arm structure or other prominent morphological features; the galaxy appears relatively smooth and undisturbed. No significant tidal features or signs of recent mergers are readily apparent. The overall impression is that of a relatively massive galaxy with low ongoing star formation.
