The galaxy appears as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. The galaxy's overall color is slightly redder, implying a population of older stars and a lower rate of ongoing star formation. The outer regions of the galaxy fade gradually into the background, indicating a less dense stellar distribution. There is no apparent spiral arm structure or significant dust lane features visible in the image. The galaxy seems relatively undisturbed, showing no clear signs of recent or ongoing mergers or tidal interactions. The structure appears mostly round, not showing a strong cigar shape.
