This galaxy appears to be a relatively smooth, though not perfectly spherical, system. The central bulge exhibits a bright, concentrated luminosity, suggesting a substantial population of older stars. Fainter, diffuse light extends outward from the bulge, indicating the presence of a galactic disk, though the features within this disk are not clearly defined, which may be caused by the viewing angle. The overall color profile appears to be skewed towards the red end of the spectrum, hinting at a population of older, redder stars and potentially, a lower ongoing star formation rate. There is a faint streak that is more visibly red to the right, which may be a result of a dust lane. The galaxy doesn't show any obvious signs of major mergers or significant tidal disturbances, though I cannot rule out minor interactions with smaller galaxies.
