The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. The overall color gradient suggests a dominance of older stellar populations, with a general redder hue. There is little evidence of spiral arm structures or significant dust lanes. The galaxy is quite compact, suggesting it is a relatively small galaxy. The light distribution is fairly uniform, indicating an absence of intense star-forming regions. There is little visual indication of any ongoing interactions or tidal disturbances affecting the galaxy's morphology.
