The galaxy presents as a roughly elliptical structure, exhibiting a smooth, gradual change in luminosity from its central region outwards. The core displays a bright, yellowish-white glow that suggests a high concentration of older stars, likely indicating an older stellar population within the galactic nucleus. Moving away from the center, the color subtly shifts towards a more reddish hue, encompassing the outer regions of the galaxy. No distinct spiral arms or prominent dust lanes are discernible in the image. The galaxy's overall morphology suggests a relatively evolved system, with little to no visible evidence of active star formation. The subtle elongation hints at a slightly flattened spheroidal shape, possibly due to rotational effects, although a lack of higher-resolution imaging makes it challenging to determine any detailed structural components.
