The galaxy presents as a relatively smooth, elliptical-like structure. The central region is notably brighter and more concentrated, exhibiting a yellowish-white hue, potentially indicating an older stellar population and reduced star formation activity. Moving outwards from the core, the light intensity gradually decreases, and the color shifts towards a slightly redder tone. The overall shape is somewhat elongated but lacks any prominent spiral arm structures or distinct morphological features. There is a very subtle, almost imperceptible distortion in the outer regions of the galaxy, suggesting a possible minor gravitational interaction or past merger event, though the galaxy appears largely undisturbed. The galaxy's light profile indicates it is a relatively evolved system, with minimal ongoing star formation.
