This galaxy presents a moderately inclined disk morphology. The central bulge is noticeable but not overly prominent, appearing somewhat diffuse and spheroidal. The galaxy exhibits signs of disturbance, possibly due to a minor interaction or internal processes. The disk displays patchy regions of differing color and luminosity, suggestive of varying stellar populations and ongoing or recent star formation. The overall color profile indicates a diverse range of stellar ages, with both bluer regions indicating younger, hotter stars, and redder regions indicating older, cooler stars. There is no clear spiral arm structure visible. The galaxy appears relatively smooth in its overall light distribution. The system's relatively low star formation rate, taken together with the presence of a smooth disk and bulge, hints at the possibility that the galaxy is in a transitional stage, possibly evolving from a more actively star-forming system.