The galaxy presents as a relatively smooth and centrally concentrated object. It appears largely elliptical in shape, with a high degree of roundness. The central region exhibits a bright, yellowish-white core, indicative of an older stellar population. Moving outward from the core, the color profile transitions to a slightly bluer hue, suggesting the presence of some younger stars, although this is minimal. There is no clear indication of spiral arm structure or a prominent disk component. The galaxy appears undisturbed, with no obvious signs of ongoing or recent merger activity.
