The galaxy presents as a relatively smooth, elliptical form, with a concentrated central bulge. The light distribution suggests a high degree of radial symmetry, with no readily apparent spiral arm structures or significant dust lanes. The core region exhibits a bright, concentrated luminosity, fading gradually towards the outer edges of the galaxy. The overall color profile indicates a population of older stars, with a subtle reddish hue suggesting the presence of evolved stellar populations. There are no obvious signs of active galactic nuclei or major star forming regions discernible in the image. The galaxy does not appear to be undergoing any major merger events, with a generally undisturbed morphology. The galaxy exhibits a slightly elongated shape, but is generally round, with a possible central bar structure.
