The observed galaxy presents as a spiral structure with a moderate inclination relative to the line of sight. Two distinct spiral arms are clearly visible, exhibiting a relatively tight winding pattern. The central bulge appears to be of moderate size.  There's an indication of a bar-like structure intersecting the bulge. The overall color profile suggests active star formation. No significant signs of ongoing major mergers or disruptive tidal interactions are apparent, although there is an indication of a minor disturbance within the galaxy's structure. The galaxy's overall form suggests it's a relatively well-defined spiral with a developed disk component.