The galaxy presents as a concentrated elliptical morphology. The core region exhibits a high surface brightness, appearing nearly spherical with a smooth, yellowish-orange hue. The light becomes more diffuse moving outward from the central bulge. This outer region maintains a roughly elliptical shape, though some very slight distortion seems to be present on one side of the galaxy. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears to be dominated by an older stellar population, given the yellow-red color and the smooth profile. The concentration of light towards the center suggests a relaxed system, consistent with an elliptical galaxy. There appears to be a low level of ongoing star formation.
