The galaxy presents as a generally elliptical morphology with a smooth, diffuse light distribution. The central region exhibits a high surface brightness, appearing almost uniformly bright and concentrated. Moving outward, the luminosity gradually decreases, with no distinct spiral arm features visible. The galaxy appears largely undisturbed, with no obvious signs of tidal tails or ongoing merger activity. Color gradients are subtle; the central region appears slightly more yellow/red, potentially indicating a higher concentration of older stellar populations, while the outer regions show a faint blue tinge, potentially indicative of some on-going star formation. The overall appearance suggests a relatively evolved system, possibly an early-type galaxy.
