The galaxy appears to be an elliptical or lenticular type. It exhibits a smooth, concentrated light profile with no apparent spiral arms or prominent dust lanes. The galaxy appears somewhat spheroidal, with a round morphology. The core region displays a brighter, more intensely colored central bulge, which appears yellowish-orange in color. This suggests an older stellar population dominating the core. The galaxy exhibits a moderately high redshift, indicating a substantial distance. There is no obvious evidence of a major ongoing merger, though subtle signs of tidal disturbances may be present upon closer inspection. Overall, the galaxy presents as a relatively quiescent system that may have a relatively low star formation rate.
