This galaxy appears to be a relatively smooth, elliptical system at a redshift of approximately 0.087, indicating a substantial distance. The central region exhibits a bright, concentrated luminosity profile, suggesting a dense stellar population, potentially an older stellar population. The galaxy's shape appears largely spheroidal, with a hint of elongation. There's a subtle color gradient visible, with the central region appearing more yellowish-white, possibly indicating an older stellar population with lower rates of star formation. The outer regions display a faint, bluish haze, perhaps indicative of younger stars or ongoing, albeit low, star formation activity. There is no clear evidence of spiral arms, a prominent disk, or major disturbances indicating recent mergers, although a minor tidal interaction cannot be ruled out based on this image alone. The overall structure suggests a galaxy with a relatively high mass.
