This galaxy appears to be a relatively smooth object with a concentrated central bulge. The galaxy exhibits a yellowish-white hue across the majority of its structure. The light distribution suggests an elliptical morphology rather than a distinct spiral pattern. There is a slight elongation, deviating slightly from a perfectly circular shape. There is no indication of a major merger event disrupting the galaxy's overall structure, although a minor disturbance cannot be entirely ruled out. Overall, the galaxy presents as a mature system with minimal evidence of ongoing, intense star formation.
