The galaxy presents as a somewhat elliptical structure, indicative of a possible early-type or lenticular morphology. A bright, concentrated central bulge is visible, exhibiting a reddish hue, which may suggest an older stellar population and/or significant dust obscuration in the core. The outer regions of the galaxy display a bluer color gradient, potentially indicating the presence of younger, hotter stars. There's a subtle hint of a disk-like structure surrounding the bulge, although the absence of well-defined spiral arms or prominent dust lanes suggests that any spiral structure is either faint or highly disrupted. The overall appearance suggests a relatively high stellar mass. The smoothness of the galaxy's light profile lends support to the classification as a smooth galaxy. Signs of disturbance, such as tidal tails or asymmetric features, are subtle but visible, possibly implying that the galaxy has recently experienced, or is still undergoing, a minor merger event.
