The galaxy presents a largely smooth morphology, with a slight elongation suggesting a flattened spheroid or possible disk component. The central region exhibits a bright, concentrated luminosity, indicative of a prominent galactic nucleus or bulge. The color profile appears relatively uniform, with a dominant yellowish-orange hue. This coloration suggests an older stellar population, with a relative scarcity of young, blue stars. There is no obvious spiral arm structure or dust lane features visible in this image. Slight disturbances may be present, but it is difficult to discern given the resolution. Overall, the galaxy appears to be an evolved system with relatively low levels of ongoing star formation.
