The galaxy presents an elliptical morphology, exhibiting a generally smooth light distribution, though with some subtle indications of internal structure or minor features that could be indicative of a disk. It appears moderately compact. The galaxy's color suggests it is likely comprised of an older stellar population, with ongoing star formation either suppressed or occurring at a low rate. There are weak signs of potential tidal disturbances or interactions, possibly indicating a previous or ongoing minor merger event.
