The galaxy appears to be a relatively smooth, elliptical type with a central, bright bulge region. The light distribution suggests a concentrated stellar population within the core, possibly indicative of an older stellar population. There may be signs of some disturbance or interaction with another object. A distinct, reddish component is visible, slightly offset from the main body of the galaxy. This may indicate a region of recent star formation, or a potential minor merger in progress. The galaxy's overall color gradient shifts from a yellowish-white center to slightly redder hues in the outer regions. The size of the galaxy is relatively compact, spanning a small angular extent in the image.
