The galaxy appears to be a single, relatively smooth object, exhibiting a centrally concentrated light profile. The overall morphology suggests an elliptical galaxy, possibly of type E3-E5 due to slight flattening. The core region displays a distinct reddish-orange hue, potentially indicative of an older stellar population. The outer regions fade gradually into the background, with a hint of a faint, extended halo. There is no obvious indication of spiral arms, a prominent disk, or tidal disturbances. The light distribution is relatively even, showing no signs of significant dust lanes or active star-forming regions within the galaxy itself.