The galaxy presents as a somewhat elliptical, smooth structure. A concentrated bulge is visually apparent, exhibiting a reddish-orange hue, indicative of a population of older stars. The outer regions of the galaxy display a gradient toward a bluer color, which may indicate the presence of younger stellar populations and ongoing, though perhaps subdued, star formation activity within the galaxy’s extended disk or halo. No distinct spiral arm structure or significant dust lanes are discernible in this image. There are no signs of major disturbances suggesting that it is undergoing a merger. Overall, the galaxy appears to be a relatively quiescent system.
