The galaxy exhibits a distinct disk morphology with an approximate diameter of around 12 arcseconds. The central region displays a high concentration of luminosity, suggesting a prominent galactic bulge or a possible active galactic nucleus. The color distribution suggests a mix of stellar populations. The central core appears blue-white, indicating a significant population of young, hot stars. The outer disk regions show a green-yellow hue, potentially indicating older stellar populations or the presence of dust lanes.

There is some visual evidence of irregularities in the galaxy's shape, possibly indicating minor gravitational interactions or ongoing merger activity. Faint extensions or tidal features may be present on one side of the galaxy. These could be the result of past or ongoing gravitational interactions with a smaller companion galaxy. Further spectroscopic and photometric data are needed to confirm the nature and extent of any such disturbances.
