The object appears to be a relatively smooth galaxy with a slight reddish hue and a centrally concentrated light profile. The galaxy's shape is nearly circular, indicating a classification leaning toward elliptical. There is a noticeable absence of distinct spiral arms or intricate features typically associated with disk galaxies. A minor disturbance or possible merging event is suggested by the asymmetry in the light distribution. Given its estimated redshift of 0.184, this is a fairly distant galaxy. The color indices, inferred from g, r, and z band magnitudes, suggest that the galaxy is likely populated by an older stellar population, with relatively low ongoing star formation.
