The galaxy presents as a relatively compact, singular object, appearing largely smooth in texture. A dominant central bulge is visible, exhibiting a bright, slightly blue-shifted coloration, suggesting a moderate level of on-going star formation in the core. There is a secondary concentration of light situated adjacent to the central bulge that may indicate an on-going disturbance of the galaxy such as tidal effects from a merger or a smaller secondary bulge, as it has a yellow-shifted coloration implying an older stellar population. There are subtle hints of potential tidal tails. Although not well defined, subtle extensions are visible near the outskirts. The overall shape appears elliptical but not perfectly circular; suggesting a relatively low disk fraction, with the majority of the light emanating from an older more central bulge.
