The galaxy presents as a somewhat elliptical, concentrated structure with a dominant central bulge. The primary color of the bulge is a yellowish-orange, suggestive of an older stellar population. A fainter, bluish region is visible on one side, hinting at the possibility of more recent star formation. The galaxy appears relatively smooth in overall texture, though there is some irregularity in the distribution of the bluer light. There are no prominent spiral arms or distinct features suggestive of a disk. The galaxy exhibits a hint of interaction or disturbance, possibly due to a minor merger or tidal interaction with a neighboring object, but the core structure remains largely undisturbed. There is also a redder point of light very close to the bluish region that could be from active star formation.
