The galaxy presents a generally smooth morphology, indicative of an elliptical or lenticular type. It exhibits a moderately elliptical shape, deviating slightly from perfect circularity. The galaxy's color profile suggests a relatively old stellar population, with a yellow-red hue dominating the central region. There is little evidence of distinct spiral arm structure or prominent dust lanes, although slight irregularities in color distribution can be seen around the edges. The central bulge appears bright and concentrated, gradually fading into the outer regions of the galaxy. There are no obvious signs of ongoing major merger activity. The galaxy's moderate redshift suggests a relatively distant location. Based on the smoothness and color characteristics, the galaxy likely possesses a substantial stellar mass and a low star formation rate.
