The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The light distribution appears centrally dominant, with a gradual falloff in surface brightness from the core outwards. There is a slight elongation, not perfectly circular but more of an in-between shape. No prominent spiral arms or distinct features are discernible in the image. The overall color profile suggests a population of older stars, giving it a yellowish hue. There is no indication of any major ongoing merger events or significant tidal disturbances, though there might be a minor hint of a disruption.
