The galaxy presents as a smooth, elliptical morphology, elongated in shape. The central region exhibits a high surface brightness, appearing as a concentrated bulge. A color gradient is observed, with the core displaying a yellowish hue, possibly indicative of an older stellar population. There is a faint, extended halo surrounding the central region. No distinct spiral arm structures or prominent dust lanes are discernible within the limitations of the image resolution. There are no signs of tidal tails or significant merger activity.
