The galaxy exhibits a somewhat elliptical morphology, appearing as a flattened spheroid when viewed from this angle. The central region is characterized by a bright, concentrated luminosity suggestive of an older stellar population, exhibiting a yellowish hue. The outer regions of the galaxy display a fainter, more diffuse light, with hints of bluish tones potentially indicative of some ongoing, but relatively low, star formation activity. There's a general lack of well-defined spiral arm structures or prominent dust lanes; the overall appearance suggests a system that is relatively smooth and evolved, lacking significant ongoing merger activity or major disturbances. While not perfectly round, the galaxy's shape leans towards an oblate spheroid rather than a highly elongated or irregular form.
