The galaxy presents as a relatively smooth, centrally concentrated object. It is generally elliptical in shape, exhibiting a high degree of roundness with only minor deviations from a perfect circle. There is a bright central bulge that appears more luminous than its surrounding stellar population. There may be some minor irregularities in its structure, possibly suggesting a past or ongoing interaction, however, there are no clear indications of a major merger event. Color gradients suggest the presence of older stellar populations. There is a slight blueing around the central bulge indicating possible star formation.
