The galaxy presents as a spiral type, with a relatively bright, concentrated central bulge. Faint spiral arms extend outwards from the bulge into a more diffuse disk. The arms exhibit a somewhat patchy structure, suggesting regions of active star formation, interspersed with areas of lower luminosity. The overall color of the bulge appears more yellow-orange, which implies an older stellar population. In contrast, the spiral arms show a hint of blue, consistent with younger, hotter stars. The galaxy is inclined relative to our line of sight, giving it an elliptical appearance. There is no strong evidence of a significant bar structure bisecting the bulge. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers with other galaxies.
