The observed galaxy exhibits a spiral morphology, viewed at a moderate inclination relative to our line of sight. A prominent central bulge is visible, displaying a yellowish hue, suggestive of an older stellar population. The disk component reveals a complex structure with two well-defined spiral arms. The spiral arms appear to be moderately wound. A prominent bar feature appears to extend through the center of the bulge. The galaxy does not display any clear signs of recent or ongoing major mergers. The overall structure suggests a relatively undisturbed, well-formed spiral galaxy.
