The galaxy presents a generally smooth and rounded morphology. The central region exhibits a high degree of luminosity, appearing significantly brighter and more concentrated than the outer regions. The light distribution decreases gradually from the center outwards, creating a diffused halo surrounding the core. There is little to no evidence of spiral arm structures or prominent dust lanes; the galaxy seems largely featureless. The color profile suggests an older stellar population, exhibiting a yellow-orange hue that may indicate lower levels of recent star formation within the galaxy. There is no indication of any major ongoing merging events or significant tidal disturbances influencing its structure. Minor asymmetry may be present, but is not clear from the image.
