The galaxy presents a generally smooth morphology, appearing as a disk-like structure seen at an oblique angle. The central region exhibits a high concentration of light, with a yellowish hue, indicative of an older stellar population. Extending outwards from the center, fainter spiral arm-like features are faintly visible, displaying bluer colors that suggest the presence of younger, hotter stars.

There is a possible indication of a minor disturbance or interaction on one side of the galaxy, with slightly disrupted or extended light distribution. Overall, the galaxy appears to be an intermediate spiral type with a dominant bulge and moderate star formation activity.
