The galaxy appears as a concentrated central body with a relatively smooth, elliptical morphology. There is little evidence of distinct spiral arms or a prominent disk structure in this image. The galaxy exhibits a yellowish-white hue, suggesting a population of older stars. A small number of faint, blueish regions can be seen near the central region which could represent regions of star formation. The light distribution is concentrated towards the center, with a gradual decline in brightness outwards. The overall appearance suggests a galaxy that is relatively evolved. There appears to be little disturbance of this object, and may not be undergoing active merging with other galaxies. The galaxy appears mostly rounded in shape.
