The galaxy appears to be a spiral type, with prominent spiral arms extending from a central bulge. The arms exhibit a patchy texture, likely indicative of active star formation regions. These regions appear bluer in color, suggesting a population of young, hot stars. Dust lanes are visible within the spiral arms, obscuring some of the starlight. 

The central bulge is relatively small and yellowish in color. A bar structure is present in the galaxy, bisecting the central bulge and extending outwards. The galaxy does not appear to be particularly smooth, with clear evidence of features such as spiral arms and dust lanes. There seems to be a second source nearby that the galaxy may be interacting with. The second source appears to be a smooth, smaller galaxy. There may be tidal distortions in this galaxy, but more data is needed to assess whether it is undergoing a major merger.
