The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The color profile suggests an older stellar population, with a dominant yellowish-orange hue indicative of evolved stars. There is a subtle color gradient visible, shifting from a slightly bluer color in the outer regions to a more pronounced yellowish hue towards the core, hinting at potential metallicity or age differences within the stellar populations. No distinct spiral arms or prominent dust lanes are visible. There is no current indication of a recent major merger event or significant tidal disturbances affecting the galaxy’s overall morphology. However, subtle asymmetrical features or faint tidal tails cannot be entirely ruled out given the image resolution. The overall smoothness suggests a morphologically early-type galaxy. 
