The galaxy appears as an elliptical or lenticular system, with a dominant spheroidal component. It exhibits a smooth, concentrated light distribution, with a high degree of central concentration and no apparent spiral arm structure or prominent dust lanes. The galaxy's color profile suggests a predominantly older stellar population, with a yellow-red hue. There is no obvious evidence of active star formation or recent merger activity. The galaxy is moderately luminous, with a semi-major axis extending roughly 3.4 kpc from the center. There may be some tidal features.
