The galaxy presents an elliptical morphology, appearing elongated and cigar-shaped in its overall form. The galaxy exhibits a smooth light distribution with a dominant central bulge. The bulge displays a yellowish-orange hue, suggesting a population of older, redder stars. Fainter and bluer light is observed on the edges of the galaxy, especially near the poles, indicative of some ongoing star formation. There are no obvious signs of spiral arms or a prominent disk component. Overall, the galaxy appears to be a relatively undisturbed system, showing no clear indication of ongoing major merging activity. The shape is consistent with an E5-E7 classification on the Hubble sequence.
