The galaxy presents as a somewhat smooth, elongated structure, approximately 5.8 kpc across its half-light radius. It exhibits a fairly uniform color gradient across its body with a possible blue shift on its upper regions. The galaxy's profile appears highly flattened, resembling a cigar shape, suggesting it is likely an elliptical galaxy viewed edge-on. There appears to be no significant sign of tidal disturbances or ongoing major mergers. Its stellar mass is estimated to be around 10^9.7 solar masses, and its star formation rate is relatively low, indicating a relatively quiescent state. The absence of prominent spiral arms or significant dust lanes further supports its classification as an elliptical galaxy. The overall color suggests a moderate population of older stars.
