The galaxy exhibits a distinct spiral structure, with two prominent arms extending from a central bulge. These arms display a moderate degree of winding. The central bulge appears relatively compact and possesses a yellowish hue, suggestive of an older stellar population. The spiral arms show a bluer coloration, likely indicating ongoing star formation activity. Overall, the galaxy demonstrates a disk-like morphology, oriented at a shallow inclination with respect to our line of sight. There is little evidence of significant interactions or mergers with other galaxies. The structure appears relatively undisturbed, maintaining a well-defined spiral pattern.
