The galaxy presents as a lenticular or early-type spiral, viewed at a significant angle, close to edge-on. It exhibits a bright, concentrated central bulge that appears largely homogenous in color, trending towards a yellow-red hue. A faint, extended disk is visible, with a bluer color than the central bulge. This suggests ongoing, albeit subdued, star formation within the disk component. No distinct spiral arm structure is discernible. The galaxy's morphology appears relatively undisturbed, with no obvious signs of recent major merger events or tidal features. The light distribution is smooth and symmetric. Overall, this galaxy likely represents a transitional object between a pure elliptical and a well-defined spiral, with a substantial spheroidal component and a relatively quiescent star formation history.
