The galaxy presents a generally smooth, elliptical morphology. A centrally concentrated bulge dominates the light profile, exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions display a redder color, which may indicate the presence of dust or a population of older, redder stars. There is minimal evidence of spiral arm structure or active star formation regions within the galaxy. The overall appearance implies a relatively evolved system, likely an elliptical galaxy observed at a considerable distance. There may be evidence of minor tidal disturbances, but it is difficult to confirm from this image.