The galaxy presents as a relatively small, moderately bright, elongated structure. It exhibits a smooth light distribution with a central bulge that is brighter compared to the outer regions. The galaxy shows a slight disk-like structure oriented approximately northeast to southwest. The color is predominantly bluish-white in the outer regions. The overall structure suggests a spiral or lenticular galaxy with a well-defined nucleus and arm-like features that are not very pronounced. There is no obvious evidence of strong tidal disturbances or ongoing major merging events. Some subtle irregularities in the outer regions might indicate minor disturbances. The presence of blue light implies recent or ongoing star formation, at least at some level.
