The galaxy presents as a relatively smooth, somewhat elongated structure, though the image resolution limits detailed morphological assessment. It exhibits a concentrated central bulge that appears to dominate the galaxy's overall light distribution. The color appears generally redder, suggesting an older stellar population and a relatively low rate of on-going star formation. There are some subtle features that might indicate a possible minor disturbance or interaction event, or perhaps an advanced merger, warranting closer inspection with higher resolution imaging. There is no obvious spiral arm structure visible. Based on the data, this galaxy appears to be in the red sequence. 