The galaxy presents as a slightly elongated structure. Its central region exhibits a bright, diffuse glow, suggesting a substantial concentration of stars. There is minimal visible structure, such as spiral arms or a prominent dust lane, indicating that it is likely a relatively smooth, featureless galaxy. The outer regions of the galaxy fade gradually into the background, lacking a sharp or well-defined edge. The color of the galaxy appears to be a yellowish-white hue, implying a stellar population dominated by older stars and a low rate of recent star formation. There might be the slight possibility of minor disturbances caused by a small merger. Overall, the galaxy's morphology is consistent with that of an elliptical galaxy.
