The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light profile. The core exhibits a bright, yellowish hue, indicative of an older stellar population, and suggests a relatively low rate of ongoing star formation. The galaxy appears mostly homogenous, lacking any distinct spiral arm structures or prominent dust lanes. A slight distortion in the galaxy's overall shape, perhaps a minor tidal disturbance, may be present, although it seems mostly undisturbed. There is the potential presence of a merging object in the lower right area of the galaxy's central bulge.
