The galaxy presents a distinct spiral structure. Two clearly defined spiral arms emanate from a central, moderately sized bulge. The arms exhibit a somewhat patchy texture, indicating regions of active star formation, likely with numerous HII regions. There is an indication of a bar-like structure running through the central bulge, although it does not appear particularly prominent. The spiral arms are relatively loosely wound. There is no obvious sign of any major merging activity or tidal disturbances, however, there are subtle irregularities that indicate possible minor interactions. The galaxy appears to be observed at a slight angle relative to face-on.
