The galaxy presents a roughly elliptical morphology, indicative of an early-type system. It exhibits a bright, concentrated central bulge, with a smooth decrease in luminosity extending outwards. The color profile suggests a mixture of stellar populations. The core displays a yellow-red hue potentially indicating an older, passively evolving population. Surrounding this core, a bluer halo may signify more recent star formation activity or the presence of a younger stellar component. The outer regions are faint and less defined, making it difficult to determine the exact extent of the galaxy. Subtle, irregular features could suggest tidal interactions, though the data is inconclusive and may also be inherent to the structure of the galaxy itself.
