The galaxy presents as a roughly elliptical form, exhibiting a concentrated central bulge that emits a yellowish-orange hue. This color suggests a stellar population dominated by older, redder stars within the bulge. The outer regions display a less intense, more diffuse light. There is very little evidence of spiral arm structure or dust lanes within the galaxy. There might be a very subtle and minor tidal disturbance or faint extension on one side of the galaxy, but there is a high degree of central concentration of light. Overall, the galaxy appears relatively smooth and featureless.
